This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA
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
Gaia DR3 4062372758160609664,2461126.9250,12.31,0.05,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 4062372758160609664 20260327.4250 12.31CV 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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:59:48.24 -29:00:00.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_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 4069668842256988800,2461126.9250,11.37,0.05,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 4069668842256988800 20260327.4250 11.37CV 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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:04:11.09 -22:28:36.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4250 2461126.9250 11.34 18:03:32.75 -24:24:58.2
5.92389 -1.16714 galactic Sgr Second-epoch detections are separated by 5.3" and 1.2 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 | Gaia DR3 4066020598282386048 | 18:03:32.01 -24:25:07.0 (Gaia DR3) | T | P | 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
Gaia DR3 4066020598282386048,2461126.9250,11.34,0.05,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 4066020598282386048 20260327.4250 11.34CV 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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:03:32.75 -24:24:58.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_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 4077588899395049088,2461126.9250,11.13,0.05,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 4077588899395049088 20260327.4250 11.13CV 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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:36:32.58 -23:52:30.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_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
V7412 Sgr,2461126.9250,11.51,0.05,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
V7412 Sgr 20260327.4250 11.51CV 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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:36:36.46 -23:53:08.3 ;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-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_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 4077190330720226688,2461126.9250,12.32,0.05,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 4077190330720226688 20260327.4250 12.32CV 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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:24:28.13 -24:54:06.3 ;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-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4250 2461126.9250 12.43 18:09:21.10 -27:44:57.2
3.64270 -3.92674 galactic Sgr Second-epoch detections are separated by 4.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J180922.32-274417.0 | 18:09:22.32 -27:44:17.0 (Gaia DR3) | SR (local) | 33.100000000000 (local) | 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
ASASSN-V J180922.32-274417.0,2461126.9250,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180922.32-274417.0 20260327.4250 12.43CV 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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:09:21.10 -27:44:57.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_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 4063395170657932544,2461126.9250,11.98,0.05,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 4063395170657932544 20260327.4250 11.98CV 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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:53:19.05 -28:19:22.8 ;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-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20_00sec_-15_00C_LIGHT_0465_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20_00sec_-14_90C_LIGHT_0219_fits__*pix.png resample_wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20_00sec_-15_00C_LIGHT_0464_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: 2461118.98182816 19.03.2026 11:33:39.953 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
First image: 2461118.98182816 19.03.2026 11:33:39.953 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Last image: 2461126.92530918 27.03.2026 10:12:16.713 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.61
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): 13427
Objects passed selection criteria: 13398
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: 11156.5
Average stars matched: 10894.2 (97.6494 %)
Memory usage VmPeak: 119720 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 06:52:19 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: 2461118.98182816 19.03.2026 11:33:39.953 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
First image: 2461118.98182816 19.03.2026 11:33:39.953 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Last image: 2461126.92530918 27.03.2026 10:12:16.713 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 98
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.27
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: 49 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): 163484
Objects passed selection criteria: 163177
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 135876
Average stars matched: 129508 (95.3134 %)
Memory usage VmPeak: 1932676 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 06:56:06 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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
SExtractor catalog cache: saved Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat to cache
SExtractor catalog cache: saved Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.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: 2461126.92470047
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits exists and is non-empty
Saving wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits to local_wcs_cache/
'wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits' -> 'local_wcs_cache/wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits'
wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits exists and is non-empty
Saving wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits to local_wcs_cache/
'wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits' -> 'local_wcs_cache/wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits'
wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits exists and is non-empty
Saving wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits to local_wcs_cache/
'wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits' -> 'local_wcs_cache/wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits'
wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits exists and is non-empty
Saving wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits to local_wcs_cache/
'wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits' -> 'local_wcs_cache/wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.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 18:14:25.391 -25:59:48.34
Second-epoch image center 18:14:25.036 -26:00:23.23
Angular distance between the image centers 0.01 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 18:14:25.391 -25:59:48.34
Second-epoch image center 18:14:24.536 -26:00:32.57
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:14:25.036 -26:00:23.23
Second-epoch second image center 18:14:24.536 -26:00:32.57
Angular distance between the image centers 0.00320 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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits &> /tmp/tmp.1qRaheaHny
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits &> /tmp/tmp.8xEXd4DWvI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits &> /tmp/tmp.qYbgtTXu4G
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits &> /tmp/tmp.qZxlyc2bKv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits and wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits and wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
Found non-empty wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits and wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
The reference image (wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits) and catalog (wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat) found
'wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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 11719 out of 16719 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.803743
a=0.000000 b=1.000000 c=22.803743
From vast_summary.log: estimated ref. image limiting mag.: -8.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.19
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.19
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
2.4 pix Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
2.7 pix fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
2.6 pix fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
Limiting magnitude estimates:
14.2 mag. Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
14.2 mag. Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
13.5 mag. fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
13.6 mag. fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 10.9 (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.1qRaheaHny (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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits' -> 'wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
WCS_IMAGE_NAME=wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
WCS-calibrated image found: wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Checking if the catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits alredy exist and is non-empty...
Catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
WCS catalog name: wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1482, passed=16719
Got 16719 stars (including 15219 good ones) from the SExtractor catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
util/solve_plate_with_UCAC5 got 16719 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 931 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: 0.69"
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 931 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: 0.83"
Excluding outliers - 916 stars left (next iteration limit 1008)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits -region wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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.8xEXd4DWvI (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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.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-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits' -> 'wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
WCS_IMAGE_NAME=wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
WCS-calibrated image found: wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
Checking if the catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits alredy exist and is non-empty...
Catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
WCS catalog name: wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1517, passed=16501
Got 16501 stars (including 14968 good ones) from the SExtractor catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat
util/solve_plate_with_UCAC5 got 16501 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 930 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: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.65"
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 917 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits -region wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.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.qYbgtTXu4G (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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
WCS-calibrated image found: wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
Checking if the catalog wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
WCS catalog name: wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=443, passed=8804
Got 8804 stars (including 8353 good ones) from the SExtractor catalog wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits.cat
util/solve_plate_with_UCAC5 got 8804 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 923 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: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
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 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.72"
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 909 stars left (next iteration limit 999)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits -region wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.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.qZxlyc2bKv (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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
WCS-calibrated image found: wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
Checking if the catalog wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
WCS catalog name: wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=478, passed=8667
Got 8667 stars (including 8184 good ones) from the SExtractor catalog wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits.cat
util/solve_plate_with_UCAC5 got 8667 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 925 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: 0.72"
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 924 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: 0.83"
Excluding outliers - 910 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits -region wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits'
Saving fully-calibrated image wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits'
Saving fully-calibrated image wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits'
Saving fully-calibrated image wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits'
Preparing the HTML report for the field Sgr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21020.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21013_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 21013_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:02:30.76 -23:00:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.70, MAG_FAINT_SEARCH_LIMIT=11.68)GAIADR2_OUTPUT=# 4.135 4069268796137510400 270.62786606017 -23.01169083706 10.5438 10.0773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21020_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 21020_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:02:28.37 -22:55:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.84, MAG_FAINT_SEARCH_LIMIT=11.82)GAIADR2_OUTPUT=# 5.278 4069270441087212544 270.61667076968 -22.93204660043 9.4830 8.1406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02527_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 02527_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:20:59.50 -29:49:39.7 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Sgr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
SExtractor catalog cache: saved Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat to cache
SExtractor catalog cache: saved Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Creating symlink local_wcs_cache/wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits exists and is non-empty
wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits exists and is non-empty
wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits exists and is non-empty
wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.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 18:14:25.391 -25:59:48.34
Second-epoch image center 18:14:25.036 -26:00:23.23
Angular distance between the image centers 0.01 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 18:14:25.391 -25:59:48.34
Second-epoch image center 18:14:24.536 -26:00:32.57
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:14:25.036 -26:00:23.23
Second-epoch second image center 18:14:24.536 -26:00:32.57
Angular distance between the image centers 0.00320 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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits &> /tmp/tmp.6TzhxVgV14
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits &> /tmp/tmp.QmK7Hy6WVb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits &> /tmp/tmp.MjZXYl2W4T
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits &> /tmp/tmp.VzrO1yRp8j
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits and wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits and wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
Found non-empty wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits and wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
The reference image (wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits) and catalog (wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat) found
'wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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 16837 out of 200125 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.519710
a=0.000000 b=1.000000 c=22.519710
From vast_summary.log: estimated ref. image limiting mag.: -8.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.25
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 69 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
2.2 pix Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
2.7 pix fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
2.5 pix fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
Limiting magnitude estimates:
14.2 mag. Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
14.3 mag. Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
13.5 mag. fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
13.6 mag. fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 12.9 (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.6TzhxVgV14 (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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits' -> 'wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
WCS_IMAGE_NAME=wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
WCS-calibrated image found: wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Checking if the catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits alredy exist and is non-empty...
Catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
WCS catalog name: wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=25986, passed=200094
Got 200094 stars (including 173914 good ones) from the SExtractor catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
util/solve_plate_with_UCAC5 got 200094 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 932 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 924 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits -region wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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.QmK7Hy6WVb (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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.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-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits' -> 'wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
WCS_IMAGE_NAME=wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
WCS-calibrated image found: wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
Checking if the catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits alredy exist and is non-empty...
Catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
WCS catalog name: wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=27503, passed=207780
Got 207780 stars (including 180064 good ones) from the SExtractor catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat
util/solve_plate_with_UCAC5 got 207780 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
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 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 926 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits -region wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.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.MjZXYl2W4T (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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
WCS-calibrated image found: wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
Checking if the catalog wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
WCS catalog name: wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=7636, passed=93053
Got 93053 stars (including 85347 good ones) from the SExtractor catalog wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits.cat
util/solve_plate_with_UCAC5 got 93053 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 922 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: 0.64"
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 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 913 stars left (next iteration limit 1002)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits -region wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.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.VzrO1yRp8j (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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
WCS-calibrated image found: wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
Checking if the catalog wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
WCS catalog name: wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=7830, passed=100245
Got 100245 stars (including 92320 good ones) from the SExtractor catalog wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits.cat
util/solve_plate_with_UCAC5 got 100245 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 923 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: 0.67"
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 922 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: 0.77"
Excluding outliers - 912 stars left (next iteration limit 1004)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Sgr-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits -region wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Saving fully-calibrated image wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
Saving fully-calibrated image wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-11-24_20.00sec_-15.00C_LIGHT_0464.fits
Saving fully-calibrated image wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.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-04-Q2b1x1_064944_TTUQ2b1x1_25482_nSt4SnaA/wcs_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465.fits
Preparing the HTML report for the field Sgr-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out234649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234934.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235036.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out235077.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out234711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53405.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 234649_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234649_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:05:51.50 -25:26:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 2.275 4065654456584134400 271.46493615707 -25.44654580285 13.2365 12.6492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234667_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234667_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:19:20.21 -28:45:10.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)
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Considering the candidate 234675_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234675_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:15:01.85 -23:59:13.6 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 234679_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234679_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:02:14.61 -21:54:53.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)
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Considering the candidate 234685_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234685_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:32:42.03 -28:20:43.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)
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Considering the candidate 234700_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234700_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:26:53.39 -23:35:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 0.531 4089444933270320512 276.72233150232 -23.58445185503 12.4885 11.4935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234702_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234702_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:18:37.29 -23:55:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 3.239 4065534266220549888 274.65585985058 -23.91705020835 12.5745 11.7295 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234707_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234707_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:05:01.46 -28:51:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.417 4050414950543818112 271.25569894222 -28.86408487463 12.1035 11.2686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234710_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234710_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:29:00.88 -25:01:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234711_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
Preparing report for the candidate 234711_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
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Considering the candidate 234713_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234713_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 234716_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234716_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:02:10.90 -28:50:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.229 4062413646058338560 270.54448196854 -28.84238343221 12.4609 11.3128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234718_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234718_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:13:49.97 -23:14:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234719_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234719_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 234720_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234720_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 17:47:18.50 -26:41:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234722_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234722_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 17:53:32.43 -24:09:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234732_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234732_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:19:49.53 -22:21:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234771_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234771_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:03:28.78 -24:23:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)GAIADR2_OUTPUT=# 2.984 4066021663424870784 270.86910866366 -24.38413128390 10.5108 9.7603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234785_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234785_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:24:35.49 -24:53:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.00, MAG_FAINT_SEARCH_LIMIT=11.98)GAIADR2_OUTPUT=# 4.808 4077189742313036160 276.14932611332 -24.88778128513 11.6314 10.6593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234795_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234795_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:20:49.33 -29:48:15.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 234796_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
Preparing report for the candidate 234796_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
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Considering the candidate 234799_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234799_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:36:10.12 -23:54:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)GAIADR2_OUTPUT=# 1.321 4077494826817553152 279.04249942599 -23.90617759939 10.8257 9.8789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234802_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
Preparing report for the candidate 234802_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
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Considering the candidate 234803_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
Preparing report for the candidate 234803_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
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Considering the candidate 234820_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234820_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 234827_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234827_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 234839_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
Preparing report for the candidate 234839_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
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Considering the candidate 234847_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234847_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:36:34.99 -23:51:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 0.694 4077589006849112832 279.14586954583 -23.85409857258 11.8716 10.9757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234877_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234877_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:02:29.75 -23:01:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 2.453 4069268791819774720 270.62323426884 -23.02002426092 12.1261 11.7899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234878_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234878_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:36:39.72 -23:52:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 5.795 4077588177831884032 279.16716233682 -23.88089067799 11.8180 11.2286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234903_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234903_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:04:11.02 -22:31:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 3.047 4069664100612365312 271.04537072192 -22.51979095001 12.1832 11.6931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234916_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234916_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 234928_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234928_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:15:05.26 -28:40:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234932_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234932_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:18:33.83 -25:36:33.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 234934_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234934_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:07:26.18 -22:05:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 2.940 4069786558719300096 271.85982216164 -22.10013965132 12.3666 11.9719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.940#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234939_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234939_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:13:03.69 -23:05:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 2.671 4066429303048323328 273.26614954169 -23.09634822753 12.2374 11.6387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234946_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234946_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:04:57.93 -25:36:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234951_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
Preparing report for the candidate 234951_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
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Considering the candidate 234975_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234975_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:33:47.61 -24:03:11.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 234998_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 234998_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 235021_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235021_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:04:18.49 -22:27:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 1.590 4069668812214688000 271.07751637774 -22.46160600025 12.7270 12.3834 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235025_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235025_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 17:53:41.08 -27:17:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235036_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235036_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:02:34.24 -24:14:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.028 4066033277018114560 270.64208567917 -24.24463570975 12.4062 11.7197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235047_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
Preparing report for the candidate 235047_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
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Considering the candidate 235048_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235048_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:10:49.31 -22:14:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 4.424 4066746344720829952 272.70676604493 -22.23682285014 12.7725 12.2699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235057_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235057_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:30:47.17 -27:57:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.708 4051597750176599168 277.69614969218 -27.95298138877 12.2458 11.4067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235060_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235060_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:32:41.32 -22:08:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235061_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235061_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:23:33.26 -23:04:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 2.040 4089512518877486592 275.88851973265 -23.07495262864 12.2020 11.0191 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235076_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235076_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:04:59.07 -23:42:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 5.635 4066170849091778304 271.24722919609 -23.71330614559 12.0033 10.8434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235077_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235077_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:03:26.42 -24:22:31.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)
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Considering the candidate 235105_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235105_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:13:30.05 -24:16:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235140_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235140_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:19:54.33 -21:44:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235144_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235144_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:07:39.85 -22:07:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235155_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235155_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:28:09.51 -26:46:51.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235171_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235171_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 235172_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235172_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 235175_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235175_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:05:55.70 -24:13:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 5.556 4066062104842243200 271.48254399700 -24.23104281287 12.8274 11.9368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235190_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235190_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 235237_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235237_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 235270_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235270_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:21:29.29 -23:26:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235288_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235288_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:05:22.42 -26:29:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235297_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235297_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:20:01.43 -23:51:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.716 4089552243071769088 275.00622868623 -23.85215760259 12.5202 11.2462 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 235305_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 235305_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 53405_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
Preparing report for the candidate 53405_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
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Considering the candidate 86981_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 86981_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:11:59.90 -27:00:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26293_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 26293_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:27:53.50 -29:47:16.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 58068_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 58068_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:08:05.10 -28:27:24.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31427_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 31427_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks
**** FOUND 18:20:59.54 -29:49:38.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 31769_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465
The candidate 31769_fd_Sgr-04-Q2b1x1_2026-03-27_05-12-16_20.00sec_-15.00C_LIGHT_0465 did not pass the final checks