This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp
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!
TCP 2026 03 22.2679* 09 54 38.68 +20 18 45.4 14.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7679,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2679 14.27CV 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/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:54:38.68 +20:18:45.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20_00sec_-14_90C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20_00sec_-14_90C_LIGHT_0146_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2679* 10 15 58.23 +19 47 22.0 13.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7679,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2679 13.07CV 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/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:15:58.23 +19:47:22.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20_00sec_-14_90C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20_00sec_-14_90C_LIGHT_0146_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2679* 10 24 29.30 +21 38 58.3 13.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7679,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2679 13.76CV 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/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:24:29.30 +21:38:58.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20_00sec_-14_90C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20_00sec_-14_90C_LIGHT_0146_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2679* 10 04 06.30 +20 03 53.9 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7679,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2679 14.07CV 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/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:04:06.30 +20:03:53.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20_00sec_-14_90C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20_00sec_-14_90C_LIGHT_0146_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2679* 09 50 57.19 +20 19 23.6 14.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7679,14.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2679 14.19CV 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/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:50:57.19 +20:19:23.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20_00sec_-14_90C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20_00sec_-14_90C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2679 2461121.7679 14.77 10:23:18.85 +22:23:26.9
212.68048 56.16201 galactic Leo Second-epoch detections are separated by 0.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J155.8283+22.3907 | 10:23:18.85 +22:23:26.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.919+/-0.091 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2679* 10 23 18.85 +22 23 26.9 14.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J155.8283+22.3907,2461121.7679,14.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J155.8283+22.3907 20260322.2679 14.77CV 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/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:23:18.85 +22:23:26.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20_00sec_-14_90C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20_00sec_-14_90C_LIGHT_0146_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2679 2461121.7679 14.84 10:22:14.10 +20:35:22.3
215.61328 55.39529 galactic Leo Second-epoch detections are separated by 5.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J155.5584+20.5894 | 10:22:14.10 +20:35:22.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.092+/-0.098 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2679* 10 22 14.10 +20 35 22.3 14.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J155.5584+20.5894,2461121.7679,14.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J155.5584+20.5894 20260322.2679 14.84CV 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/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:22:14.10 +20:35:22.3 ;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_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20_00sec_-15_00C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20_00sec_-14_90C_LIGHT_0146_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20_00sec_-14_90C_LIGHT_0146_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: 2461049.75562678 09.01.2026 06:07:56.154 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
First image: 2461049.75562678 09.01.2026 06:07:56.154 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Last image: 2461121.76822355 22.03.2026 06:26:04.515 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.80
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): 7044
Objects passed selection criteria: 7019
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 5520.75
Average stars matched: 4735.75 (85.7809 %)
Memory usage VmPeak: 112544 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 Sun Mar 22 02:13:11 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: 2461049.75562678 09.01.2026 06:07:56.154 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
First image: 2461049.75562678 09.01.2026 06:07:56.154 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Last image: 2461121.76822355 22.03.2026 06:26:04.515 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 55
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 19 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): 34250
Objects passed selection criteria: 34162
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 29262.2
Average stars matched: 26122 (89.2686 %)
Memory usage VmPeak: 134248 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 Sun Mar 22 02:14:05 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/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.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/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.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: 2461121.76762993
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits exists and is non-empty
Saving wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits to local_wcs_cache/
'wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits' -> 'local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits'
wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits exists and is non-empty
Saving wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits to local_wcs_cache/
'wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits' -> 'local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits'
wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits'
wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:14.676 +22:00:04.67
Second-epoch image center 10:09:31.193 +22:01:22.48
Angular distance between the image centers 0.07 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 10:09:14.676 +22:00:04.67
Second-epoch image center 10:09:30.110 +22:02:02.09
Angular distance between the image centers 0.07 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 10:09:31.193 +22:01:22.48
Second-epoch second image center 10:09:30.110 +22:02:02.09
Angular distance between the image centers 0.01177 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/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits &> /tmp/tmp.9aadLepQKI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits &> /tmp/tmp.5Mq07kXMBw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits &> /tmp/tmp.RUfvbJBCqa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits &> /tmp/tmp.NIY6HtJLz4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
Found non-empty wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
The reference image (wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits) and catalog (wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat) found
'wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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 3674 out of 5334 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.866726
a=0.000000 b=1.000000 c=22.866726
From vast_summary.log: estimated ref. image limiting mag.: -7.80
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.07
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
2.1 pix Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
2.5 pix fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
2.5 pix fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
Limiting magnitude estimates:
15.1 mag. Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
15.1 mag. Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
15.4 mag. fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
15.4 mag. fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.9aadLepQKI (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits' -> 'wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=391, passed=5334
Got 5334 stars (including 4935 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
util/solve_plate_with_UCAC5 got 5334 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 907 stars left (next iteration limit 997)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits -region wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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.5Mq07kXMBw (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits' -> 'wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=401, passed=5315
Got 5315 stars (including 4910 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat
util/solve_plate_with_UCAC5 got 5315 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 910 stars left (next iteration limit 1001)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits -region wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.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.RUfvbJBCqa (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_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.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_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=422, passed=7940
Got 7940 stars (including 7507 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits.cat
util/solve_plate_with_UCAC5 got 7940 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 900 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
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 900 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 900 stars left (next iteration limit 990)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits -region wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.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.NIY6HtJLz4 (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_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.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_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=429, passed=7926
Got 7926 stars (including 7487 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits.cat
util/solve_plate_with_UCAC5 got 7926 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 898 stars left (next iteration limit 988)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits -region wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.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_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits'
Saving fully-calibrated image wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits'
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits'
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits'
Preparing the HTML report for the field Leo-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20247_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 20247_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 09:47:33.69 +18:21:41.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20716_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 20716_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:07:32.31 +22:06:35.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20750_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 20750_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:12:00.07 +19:22:00.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20758_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 20758_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:09:04.43 +18:33:44.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20774_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 20774_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:10:52.06 +23:59:35.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03624_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 03624_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:07:43.42 +23:59:30.6 in the exclusion list exclusion_list.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 Leo-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Creating symlink local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.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_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits exists and is non-empty
wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits exists and is non-empty
wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits exists and is non-empty
wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:14.676 +22:00:04.67
Second-epoch image center 10:09:31.193 +22:01:22.48
Angular distance between the image centers 0.07 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 10:09:14.676 +22:00:04.67
Second-epoch image center 10:09:30.110 +22:02:02.09
Angular distance between the image centers 0.07 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 10:09:31.193 +22:01:22.48
Second-epoch second image center 10:09:30.110 +22:02:02.09
Angular distance between the image centers 0.01177 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/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits &> /tmp/tmp.DpiRAY4p5l
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits &> /tmp/tmp.HqjwlReDCO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits &> /tmp/tmp.JbryHIR2FA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits &> /tmp/tmp.8l04EoQ7hq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
Found non-empty wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
The reference image (wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits) and catalog (wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat) found
'wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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 3822 out of 30893 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.745787
a=0.000000 b=1.000000 c=22.745787
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.24
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.24
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
2.0 pix Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
2.4 pix fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
2.4 pix fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
Limiting magnitude estimates:
15.2 mag. Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
15.2 mag. Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
15.6 mag. fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
15.6 mag. fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
All-image limiting magnitude estimate: 15.6 (SNR ) 14.6 (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.DpiRAY4p5l (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits' -> 'wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1127, passed=30880
Got 30880 stars (including 29685 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
util/solve_plate_with_UCAC5 got 30880 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 902 stars left (next iteration limit 992)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits -region wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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.HqjwlReDCO (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits' -> 'wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1098, passed=31047
Got 31047 stars (including 29892 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat
util/solve_plate_with_UCAC5 got 31047 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 905 stars left (next iteration limit 995)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits -region wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.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.JbryHIR2FA (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_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.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_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1675, passed=35750
Got 35750 stars (including 34024 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits.cat
util/solve_plate_with_UCAC5 got 35750 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 893 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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
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 893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 892 stars left (next iteration limit 982)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits -region wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.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.8l04EoQ7hq (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_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.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_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=1761, passed=35524
Got 35524 stars (including 33725 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits.cat
util/solve_plate_with_UCAC5 got 35524 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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 889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 889 stars left (next iteration limit 977)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits -region wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.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_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Saving fully-calibrated image wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.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_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.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_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-25-13_20.00sec_-14.90C_LIGHT_0146.fits
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.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_2026-03-22_CI_Leo-02-Q2b1x1_021104_TTUQ2b1x1_4457_T2K8CyZp/wcs_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147.fits
Preparing the HTML report for the field Leo-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55164.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55404.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out55370.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out51917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55542.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
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 51907_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 51907_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:20:10.80 +20:14:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)GAIADR2_OUTPUT=# 2.742 625501071141650432 155.04420045281 +20.24281226378 14.9866 14.3704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51909_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 51909_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:35:31.68 +20:11:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 0.740 3987340645676920448 158.88188851245 +20.18504536846 14.6252 14.0862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51912_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 51912_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:22:34.95 +24:00:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 0.653 725734608418837760 155.64543570446 +24.01616588972 14.6862 14.2252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51917_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
Preparing report for the candidate 51917_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
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Considering the candidate 51919_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 51919_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:31:41.54 +22:57:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 0.445 722427831493885440 157.92296316071 +22.95391718170 13.7574 13.2966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53003_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
Preparing report for the candidate 53003_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
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Considering the candidate 53928_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
Preparing report for the candidate 53928_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
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Considering the candidate 54169_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
Preparing report for the candidate 54169_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
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Considering the candidate 54306_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
Preparing report for the candidate 54306_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
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Considering the candidate 54888_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 54888_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:28:20.71 +22:34:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55075_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55075_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:33:51.44 +24:57:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.53, MAG_FAINT_SEARCH_LIMIT=15.51)GAIADR2_OUTPUT=# 3.235 724353316871479808 158.46397221683 +24.96228132206 15.1770 14.3330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.235#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55164_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55164_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:00:09.37 +26:06:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 0.603 643659402595025152 150.03907247618 +26.10635974990 14.6848 14.1622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55224_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55224_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 09:54:09.03 +18:16:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 1.711 626341712205218944 148.53766384328 +18.27372384518 15.0129 14.6340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55281_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55281_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 09:46:06.51 +20:28:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.787 639629795558714752 146.52701221385 +20.47805846489 14.5697 13.9881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55364_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
Preparing report for the candidate 55364_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
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Considering the candidate 55370_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55370_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:32:36.07 +20:22:11.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)
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Considering the candidate 55384_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55384_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:12:07.02 +18:28:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.268 624896648984052608 153.02917304076 +18.47668065772 14.4275 13.5447 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55389_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55389_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:35:26.86 +25:54:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.67, MAG_FAINT_SEARCH_LIMIT=15.65)GAIADR2_OUTPUT=# 1.335 727518810848395904 158.86167305765 +25.91120098282 14.7048 14.2501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55404_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55404_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 09:55:46.10 +20:59:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.744 628129762925464704 148.94197579656 +20.99105731213 14.9185 14.3827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55423_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55423_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:30:48.12 +26:07:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 0.479 727574714142714880 157.70064451842 +26.12416448585 14.7226 13.9454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55438_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55438_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:14:42.79 +19:52:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55484_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55484_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:33:08.57 +22:34:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55488_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55488_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:28:13.54 +25:33:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 3.714 727623917288313856 157.05636362639 +25.55846947223 15.0137 14.5369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55540_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55540_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:31:59.20 +24:07:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.744 722751534588755200 157.99695136807 +24.12531326761 14.8884 14.3906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55542_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
Preparing report for the candidate 55542_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
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Considering the candidate 55556_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55556_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:27:56.71 +24:08:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.534 725792062196646016 156.98641257117 +24.14965096457 14.7749 14.2536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55561_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55561_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:33:54.82 +25:10:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 0.530 724452719594995712 158.47827693998 +25.18064696196 14.7074 14.1951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55586_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55586_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:26:59.74 +19:51:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 3.125 624585590273092096 156.74800166500 +19.86636309696 14.9301 14.3955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55627_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55627_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:27:24.90 +21:35:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 0.465 721846804022409216 156.85361134007 +21.59104645539 14.7997 14.2596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55637_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55637_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:28:26.61 +24:58:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.886 725900776408777984 157.11038354865 +24.97485922202 14.9638 14.4360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55646_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55646_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:31:05.99 +22:14:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 4.403 721523616323209472 157.77426477815 +22.24334665919 14.9432 14.4594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55648_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55648_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:35:27.05 +23:59:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.59, MAG_FAINT_SEARCH_LIMIT=15.57)GAIADR2_OUTPUT=# 0.727 724036073407810816 158.86268862503 +23.99807659911 14.6245 13.9995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55657_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55657_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:25:09.27 +25:48:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 2.130 727700917461975808 156.28798270805 +25.80670744166 14.8254 14.2702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55667_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 55667_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks
**** FOUND 10:27:20.49 +23:28:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 0.459 722655224242082688 156.83525085126 +23.47366824133 14.4749 13.6527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 29364_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147
The candidate 29364_fd_Leo-02-Q2b1x1_2026-03-22_01-26-04_20.00sec_-15.00C_LIGHT_0147 did not pass the final checks