This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky
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
ASASSN-V J185612.91-235055.5,2461126.9646,12.71,0.05,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
ASASSN-V J185612.91-235055.5 20260327.4646 12.71CV 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/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:56:13.80 -23:50:59.0 ;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_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20_00sec_-14_90C_LIGHT_0532_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20_00sec_-15_00C_LIGHT_0531_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20_00sec_-14_90C_LIGHT_0532_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20_00sec_-15_00C_LIGHT_0531_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461126.9646,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.4646 12.78CV 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/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:17:50.12 -22:37:20.7 ;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_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20_00sec_-14_90C_LIGHT_0532_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20_00sec_-15_00C_LIGHT_0531_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20_00sec_-14_90C_LIGHT_0532_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20_00sec_-15_00C_LIGHT_0531_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461126.9646,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.4646 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:02:05.91 -25:43:18.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20_00sec_-14_90C_LIGHT_0532_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20_00sec_-15_00C_LIGHT_0531_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20_00sec_-14_90C_LIGHT_0532_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20_00sec_-15_00C_LIGHT_0531_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461126.9646,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.4646 13.15CV 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/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:03:56.20 -23:32:27.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20_00sec_-14_90C_LIGHT_0532_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20_00sec_-15_00C_LIGHT_0531_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20_00sec_-14_90C_LIGHT_0532_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20_00sec_-15_00C_LIGHT_0531_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
Gaia DR3 4075409362406158848,2461126.9646,13.50,0.05,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
Gaia DR3 4075409362406158848 20260327.4646 13.50CV 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/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:57:54.14 -23:27:49.4 ;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_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20_00sec_-14_90C_LIGHT_0532_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20_00sec_-15_00C_LIGHT_0531_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20_00sec_-14_90C_LIGHT_0532_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20_00sec_-14_90C_LIGHT_0681_fits__*pix.png resample_wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20_00sec_-15_00C_LIGHT_0531_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: 2461125.96625102 26.03.2026 11:11:14.088 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
First image: 2461125.96625102 26.03.2026 11:11:14.088 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
Last image: 2461126.96484295 27.03.2026 11:09:12.431 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.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.: -8.49
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8971
Objects passed selection criteria: 8964
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 8522
Average stars matched: 8358 (98.0756 %)
Memory usage VmPeak: 115272 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 06:53:58 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: 2461125.96625102 26.03.2026 11:11:14.088 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
First image: 2461125.96625102 26.03.2026 11:11:14.088 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
Last image: 2461126.96484295 27.03.2026 11:09:12.431 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 90
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.15
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: 57 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): 96485
Objects passed selection criteria: 96396
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 90673.2
Average stars matched: 87465.5 (96.4623 %)
Memory usage VmPeak: 1883656 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 06:55:58 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/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
SExtractor catalog cache: saved Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat to cache
SExtractor catalog cache: saved Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.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/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461126.96434322
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits exists and is non-empty
Saving wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits to local_wcs_cache/
'wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits' -> 'local_wcs_cache/wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits'
wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits exists and is non-empty
Saving wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits to local_wcs_cache/
'wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits' -> 'local_wcs_cache/wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits'
wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits exists and is non-empty
Saving wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits to local_wcs_cache/
'wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits' -> 'local_wcs_cache/wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits'
wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits exists and is non-empty
Saving wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits to local_wcs_cache/
'wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits' -> 'local_wcs_cache/wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:11:56.571 -25:59:36.82
Second-epoch image center 19:12:00.675 -26:00:15.34
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:11:56.571 -25:59:36.82
Second-epoch image center 19:12:01.338 -26:00:11.86
Angular distance between the image centers 0.02 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 19:12:00.675 -26:00:15.34
Second-epoch second image center 19:12:01.338 -26:00:11.86
Angular distance between the image centers 0.00266 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/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits &> /tmp/tmp.4XeiF5SxAo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits &> /tmp/tmp.UpnjD72xWi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits &> /tmp/tmp.9MqBx7sU1y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits &> /tmp/tmp.lsXIogLEk1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.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_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits and wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.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_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits and wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat
Found non-empty wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits and wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat
The reference image (wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits) and catalog (wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat) found
'wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.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 8105 out of 10651 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.652325
a=0.000000 b=1.000000 c=22.652325
From vast_summary.log: estimated ref. image limiting mag.: -8.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.16
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.16
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
2.5 pix Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
2.6 pix fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
2.5 pix fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
Limiting magnitude estimates:
14.2 mag. Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
14.2 mag. Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
13.9 mag. fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
13.9 mag. fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.2 (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.4XeiF5SxAo (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits' -> 'wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
WCS_IMAGE_NAME=wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
WCS-calibrated image found: wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
Checking if the catalog wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits alredy exist and is non-empty...
Catalog wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
WCS catalog name: wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=714, passed=10651
Got 10651 stars (including 9923 good ones) from the SExtractor catalog wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat
util/solve_plate_with_UCAC5 got 10651 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 942 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: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 936 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits -region wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.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.UpnjD72xWi (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits' -> 'wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
WCS_IMAGE_NAME=wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
WCS-calibrated image found: wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
Checking if the catalog wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits alredy exist and is non-empty...
Catalog wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
WCS catalog name: wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=701, passed=10578
Got 10578 stars (including 9862 good ones) from the SExtractor catalog wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat
util/solve_plate_with_UCAC5 got 10578 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 944 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: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 938 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits -region wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.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.9MqBx7sU1y (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
WCS-calibrated image found: wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
Checking if the catalog wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits.cat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits.cat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
WCS catalog name: wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=471, passed=8511
Got 8511 stars (including 8028 good ones) from the SExtractor catalog wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits.cat
util/solve_plate_with_UCAC5 got 8511 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 940 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
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 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 933 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits -region wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.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.lsXIogLEk1 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
WCS-calibrated image found: wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
Checking if the catalog wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits.cat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits.cat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
WCS catalog name: wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=473, passed=8597
Got 8597 stars (including 8115 good ones) from the SExtractor catalog wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits.cat
util/solve_plate_with_UCAC5 got 8597 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 940 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
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 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 933 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits -region wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.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_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits'
Saving fully-calibrated image wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits'
Saving fully-calibrated image wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits'
Saving fully-calibrated image wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits'
Preparing the HTML report for the field Sgr-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20619.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
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 20619_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 20619_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:43:39.58 -26:14:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 0.370 4073259778514290048 280.91502531500 -26.23732816060 11.0480 10.2216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Sgr-05-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/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
SExtractor catalog cache: saved Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat to cache
SExtractor catalog cache: saved Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
Creating symlink local_wcs_cache/wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.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_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits exists and is non-empty
wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits exists and is non-empty
wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits exists and is non-empty
wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:11:56.571 -25:59:36.82
Second-epoch image center 19:12:00.675 -26:00:15.34
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:11:56.571 -25:59:36.82
Second-epoch image center 19:12:01.338 -26:00:11.86
Angular distance between the image centers 0.02 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 19:12:00.675 -26:00:15.34
Second-epoch second image center 19:12:01.338 -26:00:11.86
Angular distance between the image centers 0.00266 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/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits &> /tmp/tmp.H9hn7Wo4n5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits &> /tmp/tmp.0MTB1SsMyV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits &> /tmp/tmp.kgceOel1fK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits &> /tmp/tmp.TjuhBsnED7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.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_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits and wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.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_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits and wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat
Found non-empty wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits and wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat
The reference image (wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits) and catalog (wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat) found
'wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.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 11624 out of 108796 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.409319
a=0.000000 b=1.000000 c=22.409319
From vast_summary.log: estimated ref. image limiting mag.: -8.15
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.26
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 59 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
2.3 pix Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
2.5 pix fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
2.4 pix fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
Limiting magnitude estimates:
14.3 mag. Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
14.3 mag. Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
14.0 mag. fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
14.0 mag. fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.4 (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.H9hn7Wo4n5 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits' -> 'wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
WCS_IMAGE_NAME=wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
WCS-calibrated image found: wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
Checking if the catalog wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits alredy exist and is non-empty...
Catalog wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
WCS catalog name: wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=8591, passed=108793
Got 108793 stars (including 100032 good ones) from the SExtractor catalog wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat
util/solve_plate_with_UCAC5 got 108793 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 945 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: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits -region wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.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.0MTB1SsMyV (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits' -> 'wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
WCS_IMAGE_NAME=wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
WCS-calibrated image found: wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
Checking if the catalog wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits alredy exist and is non-empty...
Catalog wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
WCS catalog name: wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=8, blended=8843, passed=110133
Got 110133 stars (including 101112 good ones) from the SExtractor catalog wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat
util/solve_plate_with_UCAC5 got 110133 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 947 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
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 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 942 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits -region wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.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.kgceOel1fK (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
WCS-calibrated image found: wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
Checking if the catalog wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits.cat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits.cat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
WCS catalog name: wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=5596, passed=83745
Got 83745 stars (including 78036 good ones) from the SExtractor catalog wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits.cat
util/solve_plate_with_UCAC5 got 83745 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 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: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
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 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits -region wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.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.TjuhBsnED7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
WCS-calibrated image found: wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
Checking if the catalog wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits.cat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits.cat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
WCS catalog name: wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=5805, passed=85935
Got 85935 stars (including 80016 good ones) from the SExtractor catalog wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits.cat
util/solve_plate_with_UCAC5 got 85935 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 944 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 939 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits -region wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.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_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-14_20.00sec_-14.90C_LIGHT_0681.fits
Saving fully-calibrated image wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/wcs_Sgr-05-Q2b1x1_2026-03-26_06-11-57_20.00sec_-15.00C_LIGHT_0682.fits
Saving fully-calibrated image wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-08-29_20.00sec_-15.00C_LIGHT_0531.fits
Saving fully-calibrated image wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-05-Q2b1x1_065145_TTUQ2b1x1_23897_lJLaDpky/wcs_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532.fits
Preparing the HTML report for the field Sgr-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out129979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130003.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130016.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out130044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130283.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129979_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 129979_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:11:40.97 -26:23:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.039 6763243842347770368 287.92043574257 -26.38376508323 13.9866 13.3153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129980_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 129980_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:10:32.62 -29:01:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 3.995 6762309047005317504 287.63692944185 -29.02622433031 13.5371 12.8195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129985_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 129985_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:22:26.68 -28:48:14.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129987_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 129987_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:21:11.38 -26:49:19.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129989_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 129989_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:59:34.19 -26:11:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.013 4073663406668713472 284.89276954042 -26.19163169277 13.2218 12.6624 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129994_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 129994_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:21:06.64 -22:59:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.830 6770866412866492672 290.27753621293 -22.99816060149 13.6811 12.9885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129998_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 129998_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:57:52.40 -23:55:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 2.475 4075245084199866624 284.46838286724 -23.93098071521 12.9539 12.0544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130000_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130000_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:01:24.01 -22:40:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 5.264 4081469767429747072 285.35149289750 -22.67672660968 13.4371 12.7283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130003_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130003_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:10:11.89 -21:48:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 3.720 4081218219779628416 287.54963197584 -21.81605782126 13.1762 12.4679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130009_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130009_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:43:14.30 -22:47:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.005 4078508507765103360 280.80928262997 -22.78650571430 13.0842 12.2627 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130010_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130010_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:24:36.52 -29:16:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 0.474 6758695570757417600 291.15209966282 -29.26803474548 13.2003 12.8988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130016_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130016_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:55:50.31 -23:18:57.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130029_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130029_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:48:35.48 -25:29:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.121 4073206490885918464 282.14909012748 -25.48531885387 13.1031 12.3270 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130039_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130039_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130043_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130043_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:30:41.64 -23:25:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 0.326 6771391150486992640 292.67357456222 -23.42796856551 12.4334 11.5970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130044_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
Preparing report for the candidate 130044_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130050_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130050_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:20:36.67 -27:22:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.001 6765894558721847680 290.15303224101 -27.37753925405 12.3215 11.8659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130054_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130054_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130083_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130083_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130138_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
Preparing report for the candidate 130138_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130145_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
Preparing report for the candidate 130145_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130151_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130151_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:44:04.21 -23:07:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 2.486 4078355740027994624 281.01806075291 -23.13152872884 13.2527 12.3847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130166_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130166_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130171_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130171_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:43:03.05 -27:03:57.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130172_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
Preparing report for the candidate 130172_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130178_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130178_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130198_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130198_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:55:52.30 -27:00:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.018 4073525727198554752 283.96747438934 -27.01212081338 13.2859 12.7541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.018#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130218_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130218_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130232_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130232_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:19:23.67 -25:46:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 3.636 6769335377283270784 289.84762792003 -25.77673218406 13.7180 13.1276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130235_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130235_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:41:54.15 -29:59:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 0.720 4047270209853413632 280.47566680513 -29.99719662552 13.2217 12.3304 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130250_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130250_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:52:16.34 -23:35:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.915 4075500205253022336 283.06837983482 -23.59637383760 13.2566 12.4225 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130263_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130263_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:09:41.96 -29:12:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.398 6762207209045481472 287.42478282101 -29.20472387858 13.6929 13.1309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130271_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130271_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:50:13.68 -23:37:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.982 4075181037644755968 282.55658019913 -23.62561625974 11.6561 10.1911 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130283_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
Preparing report for the candidate 130283_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130284_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130284_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130285_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130285_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:44:47.36 -28:33:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.823 4071677482533434368 281.19707679126 -28.55614958896 13.7172 13.2213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130292_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130292_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:00:07.31 -28:02:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 0.866 6763357676168825088 285.03071409421 -28.04027737690 13.6032 13.1008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130298_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130298_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:08:09.70 -25:04:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.320 6764380565575028992 287.04080597722 -25.07353875776 12.8587 11.6797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130322_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130322_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:33:19.32 -26:11:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.786 6766253033871035008 293.33008008292 -26.19073918263 13.3230 12.5094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130323_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130323_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:54:59.51 -29:14:03.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130324_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130324_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:49:02.05 -24:54:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.884 4074949521728540800 282.25895812534 -24.90620635514 13.2866 12.2674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130327_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130327_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:35:02.18 -21:49:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.665 6772164970454882304 293.75957831712 -21.82644168155 13.5964 12.8640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130340_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130340_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:26:09.51 -26:23:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.283 6766020624603434240 291.53965375845 -26.38429640981 13.5781 12.8688 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130351_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130351_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:00:36.44 -29:30:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.814 6760961939101808768 285.15185570240 -29.51186454643 13.5469 12.8577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130363_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130363_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130369_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130369_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:44:35.54 -29:39:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.440 4071275125668272512 281.14805340318 -29.65934153333 13.3246 12.4866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130385_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130385_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:58:47.35 -22:22:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.753 4081688673326906752 284.69692280728 -22.37679195516 13.3466 12.5200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130387_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130387_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:31:12.19 -22:11:34.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130393_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130393_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:10:57.47 -29:07:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.499 6762304447102457984 287.73916106276 -29.12118647435 13.5480 12.8139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130399_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130399_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:24:44.72 -28:52:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.881 6758770548007170432 291.18577379650 -28.86968008230 13.4868 13.2419 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.881#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130405_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130405_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:56:25.68 -22:01:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.757 4081762198854352512 284.10700718432 -22.03365473937 13.4255 12.5894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130409_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130409_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:48:13.31 -24:09:35.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130417_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130417_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:04:53.33 -27:40:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.689 6763429075700918016 286.22250387315 -27.67394503269 13.5837 12.9169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130424_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130424_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:30:13.00 -26:16:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.661 6766215547397545856 292.55366101645 -26.26858508742 13.7109 13.2117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130447_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130447_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 18:55:41.23 -22:36:18.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130456_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130456_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:13:22.72 -29:45:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 2.124 6759206538731316352 288.34525875079 -29.76293274763 13.4779 12.9204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130461_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130461_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:30:04.16 -22:34:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.020 6771690737348348928 292.51763557180 -22.57562552045 13.9609 13.4035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130477_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130477_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks
**** FOUND 19:15:37.62 -27:40:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.010 6762878357809808512 288.90730543804 -27.67706977436 13.6282 13.0672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130492_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532
The candidate 130492_fd_Sgr-05-Q2b1x1_2026-03-27_06-09-12_20.00sec_-14.90C_LIGHT_0532 did not pass the final checks