This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2668* 11 28 15.34 +00 31 54.3 12.0 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,2461121.7668,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2668 11.96CV 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:28:15.34 +00:31:54.3 ;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-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2668* 11 07 35.84 +01 26 56.9 12.0 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,2461121.7668,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2668 12.03CV 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:07:35.84 +01:26:56.9 ;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-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2668* 11 17 09.79 +00 10 14.6 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7668,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2668 12.68CV 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:17:09.79 +00:10:14.6 ;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-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2668* 10 50 32.96 -02 19 09.7 13.4 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7668,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2668 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:50:32.96 -02:19:09.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2668* 10 59 05.22 -05 35 48.3 13.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7668,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2668 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:59:05.22 -05:35:48.3 ;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-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2668 2461121.7668 14.75 11:21:05.41 -05:41:47.0
265.93662 50.57050 galactic Leo Second-epoch detections are separated by 1.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:21:05.41 -05:41:47.0 (user input) | T | P | (position from user input) J-Ks=1.109+/-0.098 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2668* 11 21 05.41 -05 41 47.0 14.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7668,14.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2668 14.75CV 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:21:05.41 -05:41:47.0 ;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-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20_00sec_-15_00C_LIGHT_0145_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20_00sec_-14_90C_LIGHT_0144_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20_00sec_-15_00C_LIGHT_0145_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20_00sec_-14_90C_LIGHT_0144_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: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
First image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Last image: 2461121.76704649 22.03.2026 06:24:22.817 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.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.: -7.68
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): 6818
Objects passed selection criteria: 6807
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 5725.25
Average stars matched: 5225 (91.2624 %)
Memory usage VmPeak: 112552 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 03:04:38 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
First image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Last image: 2461121.76704649 22.03.2026 06:24:22.817 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 68
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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): 33645
Objects passed selection criteria: 33591
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 29283.5
Average stars matched: 27007.2 (92.2269 %)
Memory usage VmPeak: 134408 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 03:05:23 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
SExtractor catalog cache: saved Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat to cache
SExtractor catalog cache: saved Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461121.76649552
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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits exists and is non-empty
Saving wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits to local_wcs_cache/
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits exists and is non-empty
Saving wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits to local_wcs_cache/
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits exists and is non-empty
Saving wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits to local_wcs_cache/
'wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits' -> 'local_wcs_cache/wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits'
wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits exists and is non-empty
Saving wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits to local_wcs_cache/
'wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits' -> 'local_wcs_cache/wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.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 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:41.153 -01:59:07.00
Angular distance between the image centers 0.03 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 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:43.570 -01:59:17.55
Angular distance between the image centers 0.04 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 11:08:41.153 -01:59:07.00
Second-epoch second image center 11:08:43.570 -01:59:17.55
Angular distance between the image centers 0.01048 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits &> /tmp/tmp.ISe1LG14Kq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits &> /tmp/tmp.PfS9AEBrq7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits &> /tmp/tmp.YNQqnW4vbS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits &> /tmp/tmp.C8tdzrTed2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Found non-empty wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
The reference image (wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits) and catalog (wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat) found
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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 3372 out of 6399 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.879752
a=0.000000 b=1.000000 c=22.879752
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
2.2 pix Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
2.7 pix fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
2.6 pix fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
Limiting magnitude estimates:
15.2 mag. Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
15.2 mag. Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
15.2 mag. fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
15.2 mag. fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ISe1LG14Kq (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=432, passed=6399
Got 6399 stars (including 5960 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
util/solve_plate_with_UCAC5 got 6399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 947 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 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits -region wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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.PfS9AEBrq7 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=407, passed=6519
Got 6519 stars (including 6107 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
util/solve_plate_with_UCAC5 got 6519 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits -region wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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.YNQqnW4vbS (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
Checking if the catalog wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
WCS catalog name: wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=398, passed=7226
Got 7226 stars (including 6826 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits.cat
util/solve_plate_with_UCAC5 got 7226 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits -region wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.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.C8tdzrTed2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
Checking if the catalog wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
WCS catalog name: wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=428, passed=7235
Got 7235 stars (including 6798 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat
util/solve_plate_with_UCAC5 got 7235 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits -region wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
Saving fully-calibrated image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
Saving fully-calibrated image wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits'
Saving fully-calibrated image wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits'
Preparing the HTML report for the field Leo-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20863.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20841_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 20841_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20863_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 20863_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20931_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 20931_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:00:24.16 -02:42:26.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20965_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 20965_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:02:02.08 -02:30:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.033 3801783210786956032 165.50895322017 -02.50568660115 12.1713 11.6816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20988_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 20988_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:09:02.75 -05:01:17.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Leo-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:28:15.34 +00:31:54.3
11:07:35.84 +01:26:56.9
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
SExtractor catalog cache: saved Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat to cache
SExtractor catalog cache: saved Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Creating symlink local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits exists and is non-empty
wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits exists and is non-empty
wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits exists and is non-empty
wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.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 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:41.153 -01:59:07.00
Angular distance between the image centers 0.03 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 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:43.570 -01:59:17.55
Angular distance between the image centers 0.04 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 11:08:41.153 -01:59:07.00
Second-epoch second image center 11:08:43.570 -01:59:17.55
Angular distance between the image centers 0.01048 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits &> /tmp/tmp.dTYEg8DRBn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits &> /tmp/tmp.JpzHO9mtjq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits &> /tmp/tmp.6UUVoWTjiQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits &> /tmp/tmp.ruXYp360Q4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Found non-empty wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
The reference image (wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits) and catalog (wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat) found
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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 3398 out of 34371 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.774901
a=0.000000 b=1.000000 c=22.774901
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.35
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.35
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 45 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
2.2 pix Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
2.7 pix fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
2.5 pix fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
Limiting magnitude estimates:
15.4 mag. Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
15.3 mag. Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
15.3 mag. fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
15.4 mag. fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.dTYEg8DRBn (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1404, passed=34365
Got 34365 stars (including 32904 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
util/solve_plate_with_UCAC5 got 34365 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 944 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: 0.28"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits -region wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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.JpzHO9mtjq (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1420, passed=33111
Got 33111 stars (including 31640 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
util/solve_plate_with_UCAC5 got 33111 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 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: 0.30"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits -region wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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.6UUVoWTjiQ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
Checking if the catalog wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
WCS catalog name: wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1513, passed=32323
Got 32323 stars (including 30778 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits.cat
util/solve_plate_with_UCAC5 got 32323 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 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: 0.43"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits -region wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.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.ruXYp360Q4 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
Checking if the catalog wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
WCS catalog name: wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1654, passed=33769
Got 33769 stars (including 32078 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat
util/solve_plate_with_UCAC5 got 33769 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 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: 0.44"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits -region wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Saving fully-calibrated image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Saving fully-calibrated image wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-23-35_20.00sec_-14.90C_LIGHT_0144.fits
Saving fully-calibrated image wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-08-Q2b1x1_023708_TTUQ2b1x1_24410_wQAfBUVH/wcs_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145.fits
Preparing the HTML report for the field Leo-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55016.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out55536.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out55537.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out55611.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out52473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55682.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 51493_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 51493_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 10:47:47.13 -05:41:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 0.770 3776843370787014528 161.94632212480 -05.69887393505 14.6727 14.2221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51494_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 51494_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:32:21.06 -01:33:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 1.852 3793694760872124032 173.08825093713 -01.56607607082 14.3834 13.4253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51500_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 51500_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 51502_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 51502_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:14:49.15 -01:25:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 0.857 3791601290733047168 168.70492641905 -01.41736295380 14.0198 13.5284 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51504_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 51504_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:24:33.35 +00:11:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52029_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 52029_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:28:15.35 +00:31:54.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52033_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 52033_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:06:44.99 +01:57:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52069_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 52069_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:07:35.85 +01:26:56.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52473_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 52473_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
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Considering the candidate 52950_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 52950_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:29:07.36 -02:53:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52985_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 52985_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
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Considering the candidate 53520_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 53520_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:05:57.98 -05:23:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.836 3787997052961638144 166.49162760626 -05.39367237617 13.6527 13.2490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53666_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 53666_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
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Considering the candidate 54179_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 54179_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:31:31.93 -02:18:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54289_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 54289_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:26:50.79 +01:39:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54897_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 54897_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 10:45:37.10 -03:10:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 0.663 3802236179513522304 161.40448652562 -03.16881561960 14.9396 14.1081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54919_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 54919_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:23:34.29 +00:27:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 4.967 3797936848530964224 170.89416690350 +00.46092927563 14.3974 13.8412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54987_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 54987_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:06:01.47 +01:39:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 1.789 3805257427013179136 166.50623404149 +01.66590395273 14.5743 13.7487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55016_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55016_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:00:50.62 -06:05:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)GAIADR2_OUTPUT=# 4.269 3787842124901267456 165.21209260912 -06.08455316513 14.7932 14.3014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55118_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55118_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:28:30.18 -02:51:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.59, MAG_FAINT_SEARCH_LIMIT=15.57)GAIADR2_OUTPUT=# 1.447 3793443827407126912 172.12615190861 -02.85157399981 14.5542 13.9542 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 55163_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55163_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:32:19.39 +00:47:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)GAIADR2_OUTPUT=# 1.315 3797629294512772352 173.08061321405 +00.79062587000 14.5871 13.8007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55268_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55268_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:29:59.64 -00:56:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 1.392 3796792119487541888 172.49885105925 -00.93524523170 14.8014 14.2076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55300_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55300_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:31:27.25 -02:28:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 1.313 3793482933085325952 172.86364135589 -02.46779517573 14.8493 14.1952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55420_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55420_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:27:31.77 -03:42:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 1.065 3787180841672434048 171.88262676894 -03.71029508640 14.5440 13.8761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55434_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55434_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:17:03.42 +01:58:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.771 3810907581045287424 169.26464132737 +01.96895149314 14.6765 14.1786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55536_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55536_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:17:36.86 -03:10:14.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)
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Considering the candidate 55537_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55537_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:20:09.27 -03:03:23.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)
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Considering the candidate 55547_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55547_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:25:13.41 -01:28:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 0.905 3796663717145258624 171.30570626710 -01.47898025506 14.9699 14.4743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55579_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55579_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:21:00.63 -05:40:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 1.096 3786415478500536576 170.25292870550 -05.68239823943 14.7319 14.1438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55585_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55585_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:31:03.01 +01:01:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 1.503 3798402045028908032 172.76270008033 +01.02103051109 15.0430 14.5812 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55607_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55607_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:31:19.11 -01:37:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 2.234 3793690534624247424 172.83024064853 -01.62785779886 14.6084 13.8089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55611_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55611_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:20:07.44 -03:46:32.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)
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Considering the candidate 55621_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55621_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:15:12.68 -06:10:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 1.034 3784845547694734592 168.80308075262 -06.17617606846 14.7481 14.2698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55623_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55623_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:18:46.47 -06:17:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 1.854 3784865510702781696 169.69411095144 -06.28571050449 14.6875 14.2704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55627_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55627_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:26:35.04 -02:52:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 1.419 3787494614803278208 171.64579776362 -02.87725507910 15.0515 14.5105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55640_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55640_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:27:54.73 +02:09:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 1.453 3800264720805261952 171.97844462695 +02.15905458363 14.7924 14.2574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55682_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
Preparing report for the candidate 55682_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
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Considering the candidate 55697_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55697_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:28:56.65 +01:21:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 0.727 3798475025113129728 172.23610266773 +01.36372408540 14.7859 14.1073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55722_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55722_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:24:55.48 -04:11:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 1.303 3787049278234345600 171.23139591307 -04.19566373723 14.8242 14.0484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55728_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55728_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:19:48.94 +02:05:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.67, MAG_FAINT_SEARCH_LIMIT=15.65)GAIADR2_OUTPUT=# 4.294 3810736572627320704 169.95506982777 +02.09247030077 14.5704 13.9918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55782_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55782_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:27:18.56 -02:06:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 0.935 3796545897602454528 171.82751862324 -02.11387331112 14.7151 14.2205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55795_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55795_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:25:26.53 -00:21:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 1.159 3797081394124836608 171.36086211670 -00.35728167676 14.9669 14.4839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55802_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55802_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:21:40.84 +02:13:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 1.177 3810824258679824256 170.42049304596 +02.22482714232 14.2825 13.1912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55803_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55803_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks
**** FOUND 11:30:56.69 +01:49:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 1.470 3799997573839433856 172.73644624142 +01.82805400958 14.6041 13.6797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55818_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145
The candidate 55818_fd_Leo-08-Q2b1x1_2026-03-22_01-24-22_20.00sec_-15.00C_LIGHT_0145 did not pass the final checks