This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX
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 02 11.3613* 09 50 11.13 +17 02 51.6 13.0 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,2461082.8613,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260211.3613 13.01CV 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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:50:11.13 +17:02:51.6 ;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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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 02 11.3613* 10 06 59.32 +26 17 54.1 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,2461082.8613,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260211.3613 13.12CV 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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:06:59.32 +26:17:54.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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 02 11.3613* 10 15 09.35 +20 26 10.5 13.4 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,2461082.8613,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260211.3613 13.44CV 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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:15:09.35 +20:26:10.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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 02 11.3613* 09 53 00.04 +22 39 25.2 13.5 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,2461082.8613,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260211.3613 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:53:00.04 +22:39:25.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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 02 11.3613* 10 35 09.08 +17 00 07.9 13.6 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,2461082.8613,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260211.3613 13.63CV 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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:35:09.08 +17:00:07.9 ;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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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 02 11.3613* 10 23 06.50 +18 26 20.1 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,2461082.8613,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260211.3613 13.81CV 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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:23:06.50 +18:26:20.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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 02 11.3613* 10 30 43.07 +26 22 58.0 13.9 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,2461082.8613,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260211.3613 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:30:43.07 +26:22:58.0 ;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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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 02 11.3613* 10 21 32.12 +17 14 40.3 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,2461082.8613,14.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260211.3613 14.14CV 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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:21:32.12 +17:14:40.3 ;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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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 02 11.3613* 10 14 55.45 +21 32 18.9 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,2461082.8613,14.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260211.3613 14.16CV 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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:14:55.45 +21:32:18.9 ;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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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 02 11.3613* 10 31 08.86 +17 30 14.5 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,2461082.8613,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260211.3613 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:31:08.86 +17:30:14.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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 02 11.3613* 10 10 27.91 +19 50 22.3 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,2461082.8613,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260211.3613 14.33CV 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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:10:27.91 +19:50:22.3 ;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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20_00sec_-15_00C_LIGHT_0387_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20_00sec_-15_00C_LIGHT_0386_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Last image: 2461082.86175439 11.02.2026 08:40:45.579 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
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: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6517
Objects passed selection criteria: 6511
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 5949
Average stars matched: 5506 (92.5534 %)
Memory usage VmPeak: 112408 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Tue Feb 10 15:05:05 CST 2026
VaST build number 1.0rc88-299-g877bacc0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 02:43:35 CST 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-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Last image: 2461082.86175439 11.02.2026 08:40:45.579 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 168
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 11 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): 35682
Objects passed selection criteria: 35592
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 33490
Average stars matched: 31121 (92.9262 %)
Memory usage VmPeak: 136116 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Tue Feb 10 15:05:05 CST 2026
VaST build number 1.0rc88-299-g877bacc0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 02:44:25 CST 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
SExtractor catalog cache: saved Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.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: 2461082.86081083
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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits exists and is non-empty
Saving wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits to local_wcs_cache/
'wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits' -> 'local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits'
wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits exists and is non-empty
Saving wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits to local_wcs_cache/
'wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits' -> 'local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits'
wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits'
wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.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 10:09:13.999 +21:59:54.41
Angular distance between the image centers 0.00 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 10:09:11.325 +21:59:12.04
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:09:13.999 +21:59:54.41
Second-epoch second image center 10:09:11.325 +21:59:12.04
Angular distance between the image centers 0.01566 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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits &> /tmp/tmp.1tQRrxIKSm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_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-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits &> /tmp/tmp.uLFhYmkIHc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_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_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits &> /tmp/tmp.2wbjgKpIzz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits &> /tmp/tmp.d0nqSuowPy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
Found non-empty wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
The reference image (wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits) and catalog (wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat) found
'wcs_Leo-02-Q1b1x1_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.
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
____ 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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
2.1 pix Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
2.2 pix fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
2.2 pix fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
Limiting magnitude estimates:
15.1 mag. Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
15.1 mag. Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
15.3 mag. fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
15.3 mag. fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
All-image limiting magnitude estimate: 15.3 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.1tQRrxIKSm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits' -> 'wcs_Leo-02-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits -region wcs_Leo-02-Q1b1x1_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-Q1b1x1_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.uLFhYmkIHc (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits' -> 'wcs_Leo-02-Q1b1x1_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-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits -region wcs_Leo-02-Q1b1x1_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-Q1b1x1_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.2wbjgKpIzz (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_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.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_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=481, passed=6674
Got 6674 stars (including 6181 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits.cat
util/solve_plate_with_UCAC5 got 6674 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 902 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: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.37"
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_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits -region wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.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.d0nqSuowPy (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_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.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_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=467, passed=6629
Got 6629 stars (including 6149 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits.cat
util/solve_plate_with_UCAC5 got 6629 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 902 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: 0.40"
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 902 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: 0.39"
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_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits -region wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.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_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits'
Saving fully-calibrated image wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits'
Preparing the HTML report for the field Leo-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20393.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20280_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 20280_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 09:47:33.68 +18:21:23.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20378_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 20378_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:07:32.28 +22:06:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 0.391 629941891235056896 151.88439250053 +22.11007076182 12.5058 11.8501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20380_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 20380_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:16:48.90 +24:27:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.183 726386966706701184 154.20373389431 +24.45507640885 12.0425 11.3641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20388_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 20388_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:09:04.43 +18:33:44.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20393_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 20393_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:12:00.11 +19:22:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.572 625195333894472704 153.00031639484 +19.36666422949 12.2449 11.8459 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03624_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 03624_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:07:43.44 +23:59:31.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Leo-02-Q1b1x1 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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
SExtractor catalog cache: saved Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Creating symlink local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits exists and is non-empty
wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits exists and is non-empty
wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits exists and is non-empty
wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.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 10:09:13.999 +21:59:54.41
Angular distance between the image centers 0.00 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 10:09:11.325 +21:59:12.04
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:09:13.999 +21:59:54.41
Second-epoch second image center 10:09:11.325 +21:59:12.04
Angular distance between the image centers 0.01566 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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits &> /tmp/tmp.t9Qia488yu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_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-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits &> /tmp/tmp.XBVEWtjPco
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_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_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits &> /tmp/tmp.qyEW1uSD1l
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits &> /tmp/tmp.YOgk9Q1gP0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
Found non-empty wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
The reference image (wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits) and catalog (wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat) found
'wcs_Leo-02-Q1b1x1_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.
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.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.21
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.21
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 49 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
2.0 pix Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
2.0 pix fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
2.0 pix fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
Limiting magnitude estimates:
15.2 mag. Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
15.2 mag. Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
15.5 mag. fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
15.5 mag. fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
All-image limiting magnitude estimate: 15.5 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.t9Qia488yu (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits' -> 'wcs_Leo-02-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits -region wcs_Leo-02-Q1b1x1_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-Q1b1x1_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.XBVEWtjPco (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits' -> 'wcs_Leo-02-Q1b1x1_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-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits -region wcs_Leo-02-Q1b1x1_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-Q1b1x1_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.qyEW1uSD1l (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_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.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_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1605, passed=36541
Got 36541 stars (including 34864 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits.cat
util/solve_plate_with_UCAC5 got 36541 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 898 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: 0.39"
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 898 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: 0.39"
Excluding outliers - 898 stars left (next iteration limit 987)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits -region wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.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.YOgk9Q1gP0 (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_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.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_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=1552, passed=36417
Got 36417 stars (including 34802 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits.cat
util/solve_plate_with_UCAC5 got 36417 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 898 stars left (next iteration limit 987)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits -region wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.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_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.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_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-39-24_20.00sec_-15.00C_LIGHT_0386.fits
Saving fully-calibrated image wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.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_2026-02-11_CI_Leo-02-Q1b1x1_024132_TTUQ1b1x1_12653_CGF3gwAX/wcs_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387.fits
Preparing the HTML report for the field Leo-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out02553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52133.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52136.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52161.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52498.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52797.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52440.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52713.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 6s
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Considering the candidate 52128_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52128_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:40:40.76 +21:11:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52130_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52130_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:12:48.04 +22:24:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.297 629259201885553408 153.20002932642 +22.40816290963 14.5153 13.9084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52132_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52132_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:03:18.11 +25:46:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.781 738945829037126144 150.82491517773 +25.77709234138 14.0787 13.3949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52133_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52133_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:43:18.68 +26:42:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 3.569 724990724378325760 160.82744012918 +26.70423958445 14.0446 13.5380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52134_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52134_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:39:56.32 +24:05:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 2.719 723348535043116032 159.98394290752 +24.09107848304 14.1549 13.2353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52136_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52136_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 09:54:10.82 +22:37:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 0.829 641852767551869952 148.54520530588 +22.63210480617 13.3047 12.8339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52137_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52137_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:09:00.86 +26:44:38.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)
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Considering the candidate 52161_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52161_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:42:53.92 +26:33:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.25, MAG_FAINT_SEARCH_LIMIT=11.23)GAIADR2_OUTPUT=# 1.409 724987460203183872 160.72469631209 +26.55691520495 10.1719 9.8486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52272_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52272_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:42:13.88 +26:41:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 1.488 724998863340971136 160.55773941215 +26.68778979851 12.1282 11.4500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52273_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52273_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:43:25.15 +26:35:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.046 724984878927457536 160.85466140560 +26.59317819837 12.1994 11.7122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52334_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52334_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:43:31.18 +25:37:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 0.278 724678634874662272 160.87996911965 +25.62802231471 12.5842 11.8932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52348_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
Preparing report for the candidate 52348_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
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Considering the candidate 52349_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52349_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:23:52.08 +19:34:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.002 624644547289308544 155.96682150483 +19.57455592321 12.8825 12.2213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52388_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
Preparing report for the candidate 52388_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
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Considering the candidate 52416_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52416_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:43:21.58 +26:15:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 2.193 724782637507487232 160.83981749161 +26.26003631209 13.1585 12.7382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.193#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52436_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
Preparing report for the candidate 52436_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
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Considering the candidate 52440_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
Preparing report for the candidate 52440_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
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Considering the candidate 52489_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
Preparing report for the candidate 52489_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
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Considering the candidate 52498_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52498_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:43:14.46 +26:42:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.282 724990930536756096 160.80997971541 +26.71341384623 13.4424 12.8711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.282#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52513_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
Preparing report for the candidate 52513_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
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Considering the candidate 52544_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52544_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:43:26.67 +26:12:32.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)
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Considering the candidate 52560_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52560_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:10:32.40 +25:56:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 1.463 738789556652060928 152.63481755511 +25.93996148237 14.1659 13.7656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52578_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
Preparing report for the candidate 52578_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
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Considering the candidate 52591_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52591_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 09:51:59.71 +20:07:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52600_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52600_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:43:12.67 +26:27:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 1.241 724977182346521088 160.80277970079 +26.46593330612 13.9168 13.4700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52624_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52624_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 09:59:16.29 +25:10:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 2.871 642746498706373760 149.81776243296 +25.17751471832 14.1434 13.4348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52631_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52631_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:42:48.25 +26:22:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.795 724975021977896832 160.70104888181 +26.37736265191 13.9407 13.3126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52655_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
Preparing report for the candidate 52655_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
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Considering the candidate 52674_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
Preparing report for the candidate 52674_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
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Considering the candidate 52698_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52698_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:43:31.27 +26:24:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.378 724788895275053440 160.87991798649 +26.40120836239 14.0948 13.5835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52702_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
Preparing report for the candidate 52702_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
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Considering the candidate 52713_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
Preparing report for the candidate 52713_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
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Considering the candidate 52714_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52714_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:40:28.57 +26:32:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52717_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52717_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 09:54:53.26 +26:42:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 2.115 643972454171702272 148.72192244538 +26.70544019777 14.4392 13.9578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52741_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52741_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:38:58.07 +23:20:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 1.464 723167459221937024 159.74228039524 +23.34563745616 14.5846 14.0240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52746_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52746_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:42:38.09 +23:57:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52750_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52750_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:29:51.53 +19:50:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52764_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52764_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:34:26.73 +22:35:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 3.445 721638828821420544 158.61046704642 +22.58376053539 14.6564 14.2062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52781_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52781_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:40:43.30 +22:24:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52790_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52790_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:35:18.24 +26:15:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 1.794 727914600674804224 158.82552251907 +26.26613414345 14.3791 13.8095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52796_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52796_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:37:43.77 +17:07:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.764 3889685115274446336 159.43203189431 +17.11858050056 14.6424 14.2542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52797_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52797_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:40:13.70 +22:17:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 1.447 722849769080626560 160.05701859307 +22.29038018634 14.6029 14.0479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52798_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52798_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:41:11.76 +17:52:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 1.667 3985799955008495488 160.29851548320 +17.86979149913 14.5146 14.0675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52810_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52810_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:37:35.68 +26:30:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 1.480 727939477125360384 159.39831039293 +26.51510171174 14.4504 13.8699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52812_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52812_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:43:31.06 +25:35:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 1.596 724678286982059136 160.87913759496 +25.59663498477 14.3703 13.8383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52850_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52850_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 10:42:39.42 +24:02:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.564 723312045000981376 160.66401221216 +24.04854034488 14.4346 13.9330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52880_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 52880_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 02553_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 02553_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks
**** FOUND 09:37:56.87 +17:13:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 0.660 620722245714579200 144.48690480558 +17.21768500656 13.0262 12.4625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 29364_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387
The candidate 29364_fd_Leo-02-Q1b1x1_2026-02-11_02-40-45_20.00sec_-15.00C_LIGHT_0387 did not pass the final checks