This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s
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
Z Sgr,2461125.9550,11.47,0.05,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
Z Sgr 20260326.4550 11.47CV 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:19:43.41 -20:55:40.7 ;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-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.4550 2461125.9550 13.86 19:29:15.28 -13:58:00.6
24.48696 -14.59132 galactic Sgr Second-epoch detections are separated by 2.7" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J292.3142-13.9668 | 19:29:15.28 -13:58:00.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.821+/-0.076 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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
ATO J292.3142-13.9668,2461125.9550,13.86,0.05,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
ATO J292.3142-13.9668 20260326.4550 13.86CV 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:29:15.28 -13:58:00.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_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 4087952964709953408,2461125.9550,13.58,0.05,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 4087952964709953408 20260326.4550 13.58CV 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:08:31.98 -16:56:04.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_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
EF Sgr,2461125.9550,13.05,0.05,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
EF Sgr 20260326.4550 13.05CV 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:12:44.05 -14:57:16.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.9550,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.4550 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:01.94 -13:46:32.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.9550,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.4550 13.05CV 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:44:10.78 -15:36:30.5 ;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-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_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
target,2461125.9550,13.46,0.05,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
target 20260326.4550 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:46:32.98 -18:53:52.4 ;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-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.9550,13.78,0.05,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 20260326.4550 13.78CV 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:21.06 -17:18:07.4 ;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-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.9550,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.4550 13.87CV 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:22:13.48 -18:37:39.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20_00sec_-15_00C_LIGHT_0666_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20_00sec_-15_00C_LIGHT_0665_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: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461125.95522382 26.03.2026 10:55:21.338 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.53
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: 5 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): 11036
Objects passed selection criteria: 11036
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 10777.8
Average stars matched: 10093 (93.6466 %)
Memory usage VmPeak: 116500 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 05:57:23 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: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461125.95522382 26.03.2026 10:55:21.338 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 137
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.18
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: 77 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): 109016
Objects passed selection criteria: 108848
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: 105463
Average stars matched: 95305.5 (90.3689 %)
Memory usage VmPeak: 2000856 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 05:59:53 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461125.95472453
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
Saving wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits to local_wcs_cache/
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits exists and is non-empty
Saving wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits to local_wcs_cache/
'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.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 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:37.484 -17:59:57.77
Angular distance between the image centers 0.06 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 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:37.131 -18:00:04.40
Angular distance between the image centers 0.06 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 19:33:37.484 -17:59:57.77
Second-epoch second image center 19:33:37.131 -18:00:04.40
Angular distance between the image centers 0.00231 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.39Fv5YxKmw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits &> /tmp/tmp.UsWWxlNTBl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits &> /tmp/tmp.gVKByP0uza
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits &> /tmp/tmp.TsmCUYL1Pd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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 8546 out of 11017 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.784657
a=0.000000 b=1.000000 c=22.784657
From vast_summary.log: estimated ref. image limiting mag.: -8.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.25
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
2.5 pix fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
2.5 pix fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
Limiting magnitude estimates:
14.3 mag. Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
14.6 mag. Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
14.3 mag. fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
14.3 mag. fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.39Fv5YxKmw (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_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=800, passed=11017
Got 11017 stars (including 10207 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 11017 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 959 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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.UsWWxlNTBl (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/util/wcs_image_calibration.sh: line 129: echo: write error: Broken pipe
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1081, passed=13469
Got 13469 stars (including 12369 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 13469 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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.gVKByP0uza (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=733, passed=11441
Got 11441 stars (including 10702 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits.cat
util/solve_plate_with_UCAC5 got 11441 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 961 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.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.TsmCUYL1Pd (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=759, passed=11501
Got 11501 stars (including 10734 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits.cat
util/solve_plate_with_UCAC5 got 11501 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.55"
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 960 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
Saving fully-calibrated image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits'
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits'
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out22441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out22417.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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 22417_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
Preparing report for the candidate 22417_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22441_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 22441_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:35:04.93 -20:11:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 0.885 6869195359778002816 293.77028165139 -20.18416835361 11.2792 10.8635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22445_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 22445_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:39:57.38 -15:09:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 2.470 4182092364306318592 294.98840004780 -15.16174514457 11.1598 10.3422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Sgr-03-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 ####
19:19:43.41 -20:55:40.7
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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Creating symlink local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.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 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:37.484 -17:59:57.77
Angular distance between the image centers 0.06 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 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:37.131 -18:00:04.40
Angular distance between the image centers 0.06 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 19:33:37.484 -17:59:57.77
Second-epoch second image center 19:33:37.131 -18:00:04.40
Angular distance between the image centers 0.00231 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.AobWcWBH0a
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits &> /tmp/tmp.nLYpGROT3N
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits &> /tmp/tmp.xsR19Fv303
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits &> /tmp/tmp.EdhagrcTJx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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 11996 out of 101850 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.547522
a=0.000000 b=1.000000 c=22.547522
From vast_summary.log: estimated ref. image limiting mag.: -8.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.37
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 91 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
2.4 pix fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
2.4 pix fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
Limiting magnitude estimates:
14.4 mag. Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
14.7 mag. Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
14.4 mag. fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
14.4 mag. fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.7 (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.AobWcWBH0a (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_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=8404, passed=101839
Got 101839 stars (including 93311 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 101839 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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.nLYpGROT3N (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=12676, passed=138124
Got 138124 stars (including 125221 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 138124 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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.xsR19Fv303 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=8534, passed=103236
Got 103236 stars (including 94580 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits.cat
util/solve_plate_with_UCAC5 got 103236 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 962 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.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.EdhagrcTJx (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=8769, passed=106039
Got 106039 stars (including 97129 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits.cat
util/solve_plate_with_UCAC5 got 106039 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 960 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Saving fully-calibrated image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-54-38_20.00sec_-15.00C_LIGHT_0665.fits
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sgr-03-Q2b1x1_055603_TTUQ2b1x1_31905_3iLtnG7s/wcs_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666.fits
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out113268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149020.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149125.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149155.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149164.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149221.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149294.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out148971.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out148945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149395.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 20s
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: 6s
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Considering the candidate 148926_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148926_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:22:02.63 -21:40:28.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
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Considering the candidate 148929_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148929_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:18:47.39 -19:00:36.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
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Considering the candidate 148933_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148933_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:39:32.33 -14:24:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 2.901 4182915967235839360 294.88387838928 -14.41080416957 14.0344 13.3943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148942_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148942_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:32:08.53 -17:30:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.175 4179814141856297984 293.03461213546 -17.50711354551 13.8291 13.1141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148945_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
Preparing report for the candidate 148945_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
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Considering the candidate 148949_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148949_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 148950_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148950_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:37:34.02 -15:27:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.054 4181998489204897920 294.39169897733 -15.45057260334 13.9827 13.3737 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148951_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148951_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:37:23.79 -14:51:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.707 4182880885942380672 294.34834818055 -14.85768083698 13.5459 12.7553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148958_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148958_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:33:47.16 -14:25:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.534 4183056636005967104 293.44664691999 -14.42826449042 13.4394 12.4712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148961_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148961_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:45:47.73 -16:58:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.225 6871697470285291136 296.44787541659 -16.97579179472 13.9402 13.4517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148963_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148963_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:04:23.54 -20:06:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 4.996 4085374884820043008 286.09664384270 -20.10410293915 14.0351 13.3326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148964_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148964_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:08:49.00 -19:35:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 0.707 4083997750818398080 287.20416469767 -19.58961297696 13.5485 13.1110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148965_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148965_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:13:45.22 -16:25:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.144 4088055842078829440 288.43809263410 -16.42625999662 13.2606 12.5764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.144#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148969_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148969_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:19:44.64 -15:59:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.807 4183962324356578176 289.93593058931 -15.99910872120 13.8059 13.0160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148971_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148971_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:06:37.80 -20:20:30.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)
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Considering the candidate 148974_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148974_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:06:24.71 -13:51:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 2.428 4197439691225589888 286.60355728258 -13.86653618577 13.3560 12.5669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148983_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148983_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:21:47.69 -20:00:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.053 4083358487878969600 290.44762224100 -20.00077470461 14.1875 13.6495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148992_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148992_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:21:25.56 -18:17:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 0.309 4084376944884937856 290.35649386965 -18.29688657828 13.6696 13.1978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148993_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 148993_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:06:23.06 -17:15:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.878 4087568139960340224 286.59569557109 -17.25294219847 14.0043 13.4696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149010_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
Preparing report for the candidate 149010_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
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Considering the candidate 149011_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149011_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:05:22.40 -20:23:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.967 4082352640910147200 286.34336901800 -20.39926654902 13.4147 12.9221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149015_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149015_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:16:22.55 -13:45:10.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
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Considering the candidate 149018_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149018_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:06:31.07 -14:46:60.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 4.064 4089256195226077952 286.63061604713 -14.78348034320 13.3653 12.5437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149020_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149020_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:07:50.54 -16:18:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.462 4088764442969634688 286.95939567778 -16.30845927716 13.6073 13.0398 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149022_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149022_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 149024_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149024_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:52:20.60 -16:25:49.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
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Considering the candidate 149025_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149025_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:43:05.42 -18:02:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 0.519 6869918907148594048 295.77250251328 -18.03751081412 12.8748 11.9460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149026_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149026_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:14:57.18 -15:24:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.212 4184253901098955776 288.73813791520 -15.41554120930 12.8600 12.1057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149028_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149028_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:47:55.49 -20:39:42.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 149030_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149030_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:48:42.08 -16:10:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.121 6871854013253941632 297.17518296988 -16.17760928722 12.9991 12.1283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149033_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149033_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:15:21.64 -17:15:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 4.347 4087741622268150272 288.83987190663 -17.25975762838 13.1425 12.3459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149034_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149034_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:35:47.76 -17:47:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.737 4179930861885678976 293.94898324476 -17.78764849847 13.0943 12.4307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149036_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
Preparing report for the candidate 149036_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
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Considering the candidate 149039_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149039_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:07:38.49 -13:57:55.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 149041_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149041_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:10:25.39 -15:39:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 0.876 4088952047140303104 287.60604342960 -15.66553429981 12.8147 12.2899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149047_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149047_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:22:52.02 -14:52:55.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)
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Considering the candidate 149048_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149048_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:27:09.27 -20:50:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.117 6773165830974243840 291.78856145193 -20.84033233475 11.9443 11.0577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149103_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149103_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 149105_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149105_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:42:03.05 -14:06:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.661 4183297119813128192 295.51287435836 -14.11372703767 12.3199 11.4831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149125_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149125_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:15:07.14 -14:49:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.316 4185130276279001344 288.78000280716 -14.82529957834 12.5266 12.0122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149128_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149128_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 149130_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149130_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:07:38.60 -17:18:28.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)
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Considering the candidate 149134_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149134_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:24:45.10 -18:37:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 2.098 4083608042658365824 291.18736052394 -18.62794298473 12.6001 11.8840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149151_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
Preparing report for the candidate 149151_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
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Considering the candidate 149152_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149152_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:19:25.12 -18:47:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 0.343 4084261771044318720 289.85472595079 -18.78402131301 13.1497 12.6656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149155_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149155_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:37:49.56 -17:12:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.457 4180069159831438720 294.45550170758 -17.20347283321 13.2850 12.7584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149156_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
Preparing report for the candidate 149156_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
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Considering the candidate 149161_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149161_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 149162_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149162_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:06:36.40 -16:50:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 0.835 4088335495999228928 286.65161073138 -16.84530209309 13.3292 12.5643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149164_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149164_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:30:03.06 -19:22:54.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)
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Considering the candidate 149167_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149167_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:46:26.61 -19:44:31.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 149184_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149184_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:05:40.31 -18:17:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149189_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149189_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:08:11.49 -16:38:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.984 4088720904863047808 287.04760150038 -16.64170029157 13.1372 12.6808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149190_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149190_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:11:57.28 -20:13:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.573 4083713527060356224 287.98856872473 -20.22740054391 13.3709 12.8928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149201_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149201_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 149217_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149217_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:30:39.23 -21:08:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.553 6772966514433783424 292.66344498490 -21.14751456058 13.7529 13.0573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149221_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149221_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:05:11.49 -17:35:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.564 4087531890435727616 286.29774574811 -17.59093730629 13.8593 13.1011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149226_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149226_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:38:07.77 -15:32:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.844 4181985368081689472 294.53215652678 -15.53396700797 13.6976 13.2220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149233_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149233_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:11:43.58 -21:50:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.086 4081173861357836032 287.93185738773 -21.84749564562 13.8702 13.1013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149237_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
Preparing report for the candidate 149237_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
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Considering the candidate 149241_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149241_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:32:13.52 -17:05:36.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)
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Considering the candidate 149242_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149242_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:27:45.82 -18:46:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.649 4179436150372761088 291.94001186291 -18.78340298540 13.8666 13.2026 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149254_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149254_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:45:43.25 -13:46:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.422 4182674963730230528 296.43060846910 -13.77540449665 13.8503 13.2591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149262_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149262_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:13:00.77 -17:22:01.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)
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Considering the candidate 149265_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149265_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:20:59.75 -20:01:27.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
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Considering the candidate 149270_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149270_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:47:26.33 -14:34:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.174 4182385040559169664 296.86022932966 -14.56861024047 13.7172 12.9311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149272_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149272_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:05:27.57 -19:31:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.730 4085523117046098688 286.36476170701 -19.52380179860 13.6144 12.7715 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149273_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149273_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:04:42.43 -20:01:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 3.765 4085469069176592768 286.17585022007 -20.03047480407 13.6624 13.0273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149289_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149289_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:07:33.23 -22:06:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.618 4080822910990866944 286.88775619133 -22.10314719591 13.7951 13.2844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.618#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149294_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149294_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:47:55.35 -18:29:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 2.127 6869093100900256512 296.98000376865 -18.48393151896 13.8248 13.3621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149302_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149302_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:08:24.26 -17:01:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 0.833 4087950048448445312 287.10089661548 -17.01748031974 13.8874 13.4351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149317_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149317_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:39:24.49 -15:53:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.478 4181914552660507904 294.85152690281 -15.88628382652 13.8585 13.1694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149324_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149324_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:49:52.00 -14:35:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 0.881 4182329480861939840 297.46649279715 -14.58362217376 13.8563 13.1110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.881#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149347_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149347_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:16:15.00 -16:24:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.362 4087859613612235520 289.06225552611 -16.41746657740 14.2088 13.6480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149353_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
Preparing report for the candidate 149353_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
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Considering the candidate 149357_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149357_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:07:03.32 -18:32:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 2.507 4087143140036006272 286.76334025278 -18.54365507330 13.9134 13.1473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149363_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149363_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:39:52.68 -21:55:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.688 6771928953412239872 294.96915964542 -21.93126459044 13.7678 13.0385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149371_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149371_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:52:31.10 -19:35:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.103 6865735540284493056 298.12902796411 -19.60017634706 13.7035 12.9746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149374_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149374_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:06:29.10 -18:52:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 0.604 4087100435196728064 286.62142428021 -18.88233007119 14.1585 13.4245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149376_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149376_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:11:13.73 -17:58:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.670 4087272508766617088 287.80675019399 -17.97717429797 13.8895 13.3689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149379_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149379_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:06:37.63 -19:19:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.360 4085532973979977344 286.65644849854 -19.32827766588 14.2695 13.6289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149381_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149381_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:06:17.58 -20:30:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.130 4082300517185296512 286.57264253570 -20.50280095396 13.5515 12.8282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149383_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149383_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:54:18.79 -13:45:57.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)
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Considering the candidate 149388_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149388_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:06:23.84 -21:01:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.384 4082079618424322048 286.59803193991 -21.02460956892 14.0254 13.3540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149391_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149391_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 149395_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
Preparing report for the candidate 149395_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
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Considering the candidate 149416_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149416_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:12:42.08 -21:53:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.971 4081251200820761856 288.17480110504 -21.89929215227 13.7060 12.9416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149436_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149436_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:26:58.79 -21:58:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.625 6772511866376520576 291.74451825757 -21.97672384604 14.0514 13.1492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149441_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149441_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:53:23.79 -19:23:47.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)
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Considering the candidate 149452_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 149452_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks
**** FOUND 19:54:46.94 -18:53:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.304 6870286178393763584 298.69547766654 -18.90032655726 13.6791 13.0671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.304#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113268_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666
The candidate 113268_fd_Sgr-03-Q2b1x1_2026-03-26_05-55-21_20.00sec_-15.00C_LIGHT_0666 did not pass the final checks