This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461126.9939,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.4939 11.11CV 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:00:02.37 -19:34:43.3 ;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-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20_00sec_-14_90C_LIGHT_0562_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20_00sec_-14_90C_LIGHT_0561_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20_00sec_-14_90C_LIGHT_0562_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20_00sec_-14_90C_LIGHT_0561_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4939 2461126.9939 12.97 19:00:26.24 -13:47:15.4
21.58607 -8.19852 galactic Sgr Second-epoch detections are separated by 1.1" and 2.2 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 J285.1083-13.7857 | 19:00:27.06 -13:47:26.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
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 J285.1083-13.7857,2461126.9939,12.97,0.05,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 J285.1083-13.7857 20260327.4939 12.97CV 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:00:26.24 -13:47:15.4 ;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-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20_00sec_-14_90C_LIGHT_0562_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20_00sec_-14_90C_LIGHT_0561_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20_00sec_-14_90C_LIGHT_0562_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20_00sec_-14_90C_LIGHT_0561_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 4091862316976633984,2461126.9939,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4091862316976633984 20260327.4939 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:31:27.37 -20:40:38.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20_00sec_-14_90C_LIGHT_0562_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20_00sec_-14_90C_LIGHT_0561_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20_00sec_-14_90C_LIGHT_0562_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20_00sec_-14_90C_LIGHT_0561_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461126.9939,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.4939 12.41CV 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:59:05.87 -19:10:05.8 ;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-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20_00sec_-14_90C_LIGHT_0562_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20_00sec_-14_90C_LIGHT_0561_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20_00sec_-14_90C_LIGHT_0562_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20_00sec_-14_90C_LIGHT_0561_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.4939* 18 19 23.67 -14 05 44.3 12.6 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4146400533244936448,2461126.9939,12.55,0.05,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 4146400533244936448 20260327.4939 12.55CV 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:19:23.67 -14:05:44.3 ;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-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20_00sec_-14_90C_LIGHT_0562_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20_00sec_-14_90C_LIGHT_0561_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20_00sec_-14_90C_LIGHT_0562_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20_00sec_-14_90C_LIGHT_0200_fits__*pix.png resample_wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20_00sec_-14_90C_LIGHT_0561_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: 2461118.95649310 19.03.2026 10:57:11.004 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
First image: 2461118.95649310 19.03.2026 10:57:11.004 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Last image: 2461126.99419859 27.03.2026 11:51:28.758 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.46
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15272
Objects passed selection criteria: 15241
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 12693.5
Average stars matched: 12064.5 (95.0447 %)
Memory usage VmPeak: 121604 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 07:48:02 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: 2461118.95649310 19.03.2026 10:57:11.004 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
First image: 2461118.95649310 19.03.2026 10:57:11.004 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Last image: 2461126.99419859 27.03.2026 11:51:28.758 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 121
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.06
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: 63 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): 171290
Objects passed selection criteria: 171007
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 148913
Average stars matched: 140220 (94.162 %)
Memory usage VmPeak: 2239556 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 07:51:31 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
SExtractor catalog cache: saved Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat to cache
SExtractor catalog cache: saved Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461126.99366421
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits exists and is non-empty
Saving wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits to local_wcs_cache/
'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits' -> 'local_wcs_cache/wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits'
wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits exists and is non-empty
Saving wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits to local_wcs_cache/
'wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits' -> 'local_wcs_cache/wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits'
wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits exists and is non-empty
Saving wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits to local_wcs_cache/
'wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits' -> 'local_wcs_cache/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits'
wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits exists and is non-empty
Saving wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits to local_wcs_cache/
'wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits' -> 'local_wcs_cache/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.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 18:40:02.901 -17:59:22.60
Second-epoch image center 18:40:13.038 -18:00:49.16
Angular distance between the image centers 0.05 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 18:40:02.901 -17:59:22.60
Second-epoch image center 18:40:13.955 -18:00:46.82
Angular distance between the image centers 0.05 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 18:40:13.038 -18:00:49.16
Second-epoch second image center 18:40:13.955 -18:00:46.82
Angular distance between the image centers 0.00369 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits &> /tmp/tmp.r8GBhSKQsn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits &> /tmp/tmp.ymF841jLlM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits &> /tmp/tmp.bvCZX4pbYb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits &> /tmp/tmp.SI5pjrFuVV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
Found non-empty wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
The reference image (wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits) and catalog (wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat) found
'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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 12239 out of 18356 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.804368
a=0.000000 b=1.000000 c=22.804368
From vast_summary.log: estimated ref. image limiting mag.: -8.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.34
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
2.1 pix Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
2.5 pix fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
2.6 pix fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
Limiting magnitude estimates:
14.3 mag. Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
14.5 mag. Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
13.8 mag. fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
13.7 mag. fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.0 (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.r8GBhSKQsn (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits' -> 'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS-calibrated image found: wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Checking if the catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS catalog name: wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1700, passed=18356
Got 18356 stars (including 16644 good ones) from the SExtractor catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
util/solve_plate_with_UCAC5 got 18356 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 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: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.73"
Estimated accuracy of the plate solution: 0.82"
Excluding outliers - 939 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits -region wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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.ymF841jLlM (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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits' -> 'wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS-calibrated image found: wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Checking if the catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS catalog name: wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1941, passed=20338
Got 20338 stars (including 18376 good ones) from the SExtractor catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat
util/solve_plate_with_UCAC5 got 20338 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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 938 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits -region wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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.bvCZX4pbYb (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
Checking if the catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
WCS catalog name: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=893, passed=10254
Got 10254 stars (including 9354 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits.cat
util/solve_plate_with_UCAC5 got 10254 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 937 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: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 929 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits -region wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.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.SI5pjrFuVV (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
Checking if the catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
WCS catalog name: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=826, passed=9769
Got 9769 stars (including 8941 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits.cat
util/solve_plate_with_UCAC5 got 9769 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 939 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: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.70"
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits -region wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits'
Saving fully-calibrated image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits'
Saving fully-calibrated image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits'
Saving fully-calibrated image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits'
Preparing the HTML report for the field Sgr-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out22497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out22508.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22497_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 22497_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:35:31.50 -13:56:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 0.669 4104507658467518080 278.88107222974 -13.94434770399 11.3086 10.9201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22508_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
Preparing report for the candidate 22508_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Sgr-02-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 ####
19:00:02.37 -19:34:43.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
SExtractor catalog cache: saved Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat to cache
SExtractor catalog cache: saved Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Creating symlink local_wcs_cache/wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits exists and is non-empty
wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits exists and is non-empty
wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits exists and is non-empty
wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.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 18:40:02.901 -17:59:22.60
Second-epoch image center 18:40:13.038 -18:00:49.16
Angular distance between the image centers 0.05 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 18:40:02.901 -17:59:22.60
Second-epoch image center 18:40:13.955 -18:00:46.82
Angular distance between the image centers 0.05 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 18:40:13.038 -18:00:49.16
Second-epoch second image center 18:40:13.955 -18:00:46.82
Angular distance between the image centers 0.00369 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits &> /tmp/tmp.CoCcNuP5vQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits &> /tmp/tmp.5a83LoNSOz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits &> /tmp/tmp.T0Z6RES8eA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits &> /tmp/tmp.GgQT1ucILD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
Found non-empty wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
The reference image (wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits) and catalog (wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat) found
'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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 16072 out of 204414 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.510618
a=0.000000 b=1.000000 c=22.510618
From vast_summary.log: estimated ref. image limiting mag.: -8.06
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 98 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
2.1 pix Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
2.3 pix fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
2.4 pix fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
Limiting magnitude estimates:
14.5 mag. Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
14.6 mag. Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
13.9 mag. fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
13.8 mag. fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.CoCcNuP5vQ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits' -> 'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS-calibrated image found: wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Checking if the catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS catalog name: wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=37, blended=26568, passed=204377
Got 204377 stars (including 177585 good ones) from the SExtractor catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
util/solve_plate_with_UCAC5 got 204377 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits -region wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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.5a83LoNSOz (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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits' -> 'wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS-calibrated image found: wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Checking if the catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS catalog name: wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=30504, passed=224228
Got 224228 stars (including 193440 good ones) from the SExtractor catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat
util/solve_plate_with_UCAC5 got 224228 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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 939 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits -region wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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.T0Z6RES8eA (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
Checking if the catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
WCS catalog name: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=10195, passed=121350
Got 121350 stars (including 111035 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits.cat
util/solve_plate_with_UCAC5 got 121350 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
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 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.62"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits -region wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.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.GgQT1ucILD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
Checking if the catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
WCS catalog name: wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=9290, passed=111744
Got 111744 stars (including 102337 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits.cat
util/solve_plate_with_UCAC5 got 111744 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 939 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: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.62"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits -region wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Saving fully-calibrated image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Saving fully-calibrated image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-50-42_20.00sec_-14.90C_LIGHT_0561.fits
Saving fully-calibrated image wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-02-Q2b1x1_074550_TTUQ2b1x1_28197_hkSUmdUy/wcs_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562.fits
Preparing the HTML report for the field Sgr-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out248272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248404.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out248438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248601.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
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: 2s
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Considering the candidate 248272_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248272_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:46:49.93 -19:44:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.464 4086196121269261824 281.70805494129 -19.73623236505 13.4503 12.6387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248283_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248283_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:35:25.32 -17:37:44.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)
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Considering the candidate 248298_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248298_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:57:51.75 -16:20:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.610 4100577046156593664 284.46534358880 -16.34328230305 13.0685 12.2016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248303_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248303_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 19:05:22.81 -14:57:31.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
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Considering the candidate 248316_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248316_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:13:57.16 -19:32:05.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)
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Considering the candidate 248342_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248342_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:45:18.30 -18:30:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.340 4098396126153566592 281.32611912569 -18.50401031412 13.0858 12.1186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.340#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248345_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248345_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:16:41.31 -14:50:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248346_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248346_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:53:23.61 -14:09:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248349_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248349_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:34:55.76 -15:51:47.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 248371_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248371_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:24:33.65 -14:33:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 1.763 4104267075896975232 276.14068999006 -14.55679475304 13.0490 12.1890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248377_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248377_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:18:45.35 -17:10:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.630 4097316268292451584 274.68972298894 -17.17518719202 12.9224 12.4828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248379_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248379_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:55:21.36 -16:14:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 0.871 4100614837536488064 283.83877492100 -16.23408541025 13.3833 12.5580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248403_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248403_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:28:06.81 -15:15:03.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)
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Considering the candidate 248404_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248404_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:15:17.73 -16:20:28.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)
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Considering the candidate 248406_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248406_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:24:03.14 -20:45:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248408_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248408_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:33:55.20 -16:23:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248409_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248409_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:12:21.35 -21:50:47.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)
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Considering the candidate 248412_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248412_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:54:28.39 -18:21:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 2.473 4086776418554021376 283.61766911814 -18.35587182061 12.8518 12.0959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248426_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248426_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:44:10.66 -21:55:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 1.576 4079328223704682368 281.04396531718 -21.91987244463 13.0832 12.2837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248431_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248431_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:45:51.10 -17:18:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248432_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248432_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:30:44.40 -16:52:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248438_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
Preparing report for the candidate 248438_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
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Considering the candidate 248439_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248439_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:59:36.12 -15:57:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248444_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
Preparing report for the candidate 248444_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
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Considering the candidate 248454_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248454_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:48:47.68 -20:23:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 3.269 4079957522312291968 282.19961107168 -20.39923070917 12.2835 11.0687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248460_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248460_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:59:56.36 -13:47:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248461_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248461_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:49:04.53 -20:35:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248462_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248462_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:12:14.52 -15:24:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248465_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248465_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 19:01:41.36 -14:04:27.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)
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Considering the candidate 248466_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248466_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 19:00:15.45 -19:49:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248476_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248476_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:18:55.83 -18:06:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.229 4096392815964107264 274.73278457546 -18.10983301872 12.2613 11.7816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248478_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248478_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:28:57.88 -14:13:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 5.871 4104337199798682240 277.23949805648 -14.22559762367 12.0195 11.5746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248479_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248479_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:39:12.27 -16:54:41.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)
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Considering the candidate 248480_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248480_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:18:05.90 -18:44:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248484_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248484_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:14:35.08 -18:48:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248485_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248485_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:40:15.10 -15:13:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248486_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248486_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:48:20.84 -19:12:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248487_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248487_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:17:14.51 -18:16:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.843 4096397699445951616 274.31067374934 -18.27516371211 12.3720 11.8770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248488_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248488_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 19:05:26.63 -17:53:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.173 4087416162522608128 286.36105655828 -17.88782039499 12.2474 11.4897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248494_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248494_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:36:48.13 -17:13:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248496_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248496_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:53:52.35 -21:12:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248499_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248499_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:21:28.80 -16:51:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 1.320 4097354308830988416 275.36961833029 -16.86491171169 11.6249 10.5858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248504_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248504_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 19:02:31.94 -18:41:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 1.443 4085858498138046080 285.63307854341 -18.69059912356 11.6540 10.8730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248508_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248508_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:42:12.93 -20:42:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 0.408 4080085551047454464 280.55379972752 -20.70630003441 11.1180 10.4949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248510_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248510_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 19:02:58.13 -15:45:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.63, MAG_FAINT_SEARCH_LIMIT=11.61)GAIADR2_OUTPUT=# 0.046 4089077357111022976 285.74221826713 -15.75938033352 10.4788 9.7323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248528_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248528_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:19:44.06 -18:10:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 1.413 4096411099745642496 274.93377436147 -18.16917965322 12.0803 11.6058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248537_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248537_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:57:39.94 -21:08:16.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 248542_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248542_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:53:34.95 -17:47:35.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)
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Considering the candidate 248543_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248543_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:42:58.88 -19:14:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248551_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248551_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:15:26.95 -18:40:33.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248556_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248556_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:17:16.92 -17:20:48.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248568_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248568_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:15:08.27 -20:44:34.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248569_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248569_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:14:49.79 -18:48:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248571_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248571_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:13:45.37 -21:01:33.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 248574_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248574_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:15:10.43 -18:59:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248578_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
Preparing report for the candidate 248578_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
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Considering the candidate 248584_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248584_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:54:35.93 -15:36:06.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248595_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248595_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:38:55.94 -15:02:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 2.763 4103425601574580608 279.73228874850 -15.04948975194 12.4560 11.8693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248596_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248596_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:49:39.35 -19:09:45.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248600_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248600_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:32:23.75 -18:57:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 4.057 4093286283304403328 278.09824461843 -18.95845863473 12.3873 11.4420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248601_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
Preparing report for the candidate 248601_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
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Considering the candidate 248604_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248604_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 248605_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248605_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:27:28.09 -15:21:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248611_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248611_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:35:27.38 -20:50:39.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248612_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248612_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:52:33.71 -16:41:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.544 4099104112897532160 283.14002156515 -16.68996068038 12.8842 12.2743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248613_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248613_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:58:50.64 -15:33:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 1.403 4100779008373088256 284.71135961418 -15.55465474710 11.5249 10.1118 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248618_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248618_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:25:01.42 -18:30:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 4.728 4096185317506436480 276.25577588810 -18.51211016332 12.9937 12.5402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248620_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248620_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:32:24.99 -18:57:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 4.587 4093286283304426368 278.10424121070 -18.95486951279 12.1242 10.9793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248621_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248621_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:15:04.60 -20:51:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 3.974 4093954344031725952 273.76928736259 -20.85420742916 12.7719 12.2471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248623_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248623_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:55:39.03 -20:02:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.211 4085273661031250944 283.91249040804 -20.03682713704 12.5936 12.0729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248624_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248624_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:48:16.31 -14:42:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248626_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248626_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:58:33.50 -19:11:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248629_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248629_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:45:21.85 -20:37:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 3.112 4080122831350117376 281.34096523495 -20.63144397907 12.8188 12.3043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248632_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248632_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:11:16.07 -19:26:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248633_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248633_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:24:09.41 -19:24:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 3.161 4093025084967653504 276.04007644066 -19.40321087406 12.5608 11.5891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248635_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248635_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:36:44.59 -17:14:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.227 4099697844844025216 279.18541001514 -17.23479112718 12.4793 11.6141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248636_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248636_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:28:02.36 -21:35:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 0.688 4090281936499075072 277.00994764049 -21.59900793814 12.4347 11.3866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248640_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248640_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:11:51.90 -20:21:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248646_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248646_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:19:46.47 -17:44:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248655_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248655_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:29:40.15 -16:39:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248657_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248657_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:31:32.40 -14:16:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248660_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248660_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:55:27.91 -16:23:56.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248661_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248661_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:12:14.48 -17:23:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.397 4095951022752862464 273.05993253984 -17.39277099071 13.1814 12.8291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248664_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248664_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:50:58.74 -15:15:11.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)
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Considering the candidate 248665_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248665_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:13:36.40 -19:12:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248676_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248676_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:40:32.39 -16:59:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 2.481 4099632634423691520 280.13461211727 -16.99420118087 13.3408 12.7975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248697_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248697_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:54:27.70 -18:09:39.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
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Considering the candidate 248701_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248701_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:45:56.50 -17:45:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248703_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248703_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:48:40.03 -18:41:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.290 4086415336399986048 282.16655362405 -18.69398861933 13.0783 12.2043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248709_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248709_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:26:35.06 -14:38:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248719_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248719_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:55:57.62 -17:35:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 4.585 4086958117174547072 283.99030892764 -17.58938350148 12.8114 11.9999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248721_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248721_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:56:25.20 -19:16:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248723_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248723_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:25:53.67 -17:03:49.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 248734_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248734_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:34:07.16 -19:47:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248752_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248752_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:29:40.66 -18:23:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248803_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248803_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:55:15.45 -20:09:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.550 4085270774815035392 283.81435946891 -20.15881966842 13.4629 12.4707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248857_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 248857_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks
**** FOUND 18:40:54.93 -17:08:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.104 4099614488149080576 280.22905788725 -17.14816481479 13.7184 12.7405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65821_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562
The candidate 65821_fd_Sgr-02-Q2b1x1_2026-03-27_06-51-28_20.00sec_-14.90C_LIGHT_0562 did not pass the final checks