This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.3752* 10 52 52.05 +10 53 02.3 10.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.8752,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.3752 10.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:52:52.05 +10:53:02.3 ;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-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.3752* 10 22 53.94 +12 12 12.0 11.7 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,2461083.8752,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.3752 11.67CV 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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:22:53.94 +12:12:12.0 ;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-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.3752* 11 02 43.21 +10 15 46.0 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,2461083.8752,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.3752 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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:02:43.21 +10:15:46.0 ;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-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.3752* 10 12 17.34 +15 29 24.9 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.8752,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.3752 12.54CV 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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:12:17.34 +15:29:24.9 ;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-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.3752* 10 57 56.31 +09 23 14.6 12.8 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
IU Leo,2461083.8752,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IU Leo 20260212.3752 12.82CV 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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:57:56.31 +09:23:14.6 ;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-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.3752* 10 53 35.22 +18 05 32.8 12.8 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,2461083.8752,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.3752 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:53:35.22 +18:05:32.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.3752* 10 22 13.75 +18 31 02.8 13.7 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,2461083.8752,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.3752 13.73CV 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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:22:13.75 +18:31:02.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.3752* 10 34 19.70 +17 06 39.0 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,2461083.8752,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.3752 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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:34:19.70 +17:06:39.0 ;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-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.3752* 10 20 48.17 +17 20 46.1 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.8752,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.3752 14.05CV 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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:20:48.17 +17:20:46.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.3752* 10 14 49.44 +14 41 54.4 14.0 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,2461083.8752,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.3752 14.04CV 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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:14:49.44 +14:41:54.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.3752* 10 42 50.73 +12 03 05.5 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.8752,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.3752 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:42:50.73 +12:03:05.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.3752* 10 10 20.30 +11 44 18.5 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.8752,14.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.3752 14.36CV 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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:10:20.30 +11:44:18.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.3752* 10 57 32.54 +10 49 46.7 14.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.8752,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.3752 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:57:32.54 +10:49:46.7 ;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-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.3752* 10 30 13.98 +17 31 24.0 14.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.8752,14.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.3752 14.47CV 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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:30:13.98 +17:31:24.0 ;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-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.3752 2461083.8752 11.89 11:11:05.83 +18:40:24.1
227.75402 65.45093 galactic Leo Second-epoch detections are separated by 0.6" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3984034719154051456 | 11:11:05.75 +18:40:23.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.638+/-0.031 (K)
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 02 12.3752* 11 11 05.83 +18 40 24.1 11.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3984034719154051456,2461083.8752,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3984034719154051456 20260212.3752 11.89CV 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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:11:05.83 +18:40:24.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20_00sec_-15_00C_LIGHT_0421_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20_00sec_-15_00C_LIGHT_0402_fits__*pix.png resample_wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20_00sec_-14_90C_LIGHT_0420_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: 2461058.87067979 18.01.2026 08:53:36.734 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
First image: 2461058.87067979 18.01.2026 08:53:36.734 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
Last image: 2461083.87549709 12.02.2026 09:00:32.949 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.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.: -7.53
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): 6622
Objects passed selection criteria: 6617
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 6326.25
Average stars matched: 6115 (96.6607 %)
Memory usage VmPeak: 115692 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Feb 12 03:04:30 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.87067979 18.01.2026 08:53:36.734 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
First image: 2461058.87067979 18.01.2026 08:53:36.734 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
Last image: 2461083.87549709 12.02.2026 09:00:32.949 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 111
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
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: 10 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): 35229
Objects passed selection criteria: 35125
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 33920.5
Average stars matched: 32623.8 (96.1771 %)
Memory usage VmPeak: 136228 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Feb 12 03:05:28 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
SExtractor catalog cache: saved Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat to cache
SExtractor catalog cache: saved Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.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: 2461083.87488627
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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits exists and is non-empty
Saving wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits to local_wcs_cache/
'wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits' -> 'local_wcs_cache/wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits'
wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits exists and is non-empty
Saving wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits to local_wcs_cache/
'wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits' -> 'local_wcs_cache/wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits'
wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits exists and is non-empty
Saving wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits to local_wcs_cache/
'wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits' -> 'local_wcs_cache/wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits'
wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits exists and is non-empty
Saving wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits to local_wcs_cache/
'wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits' -> 'local_wcs_cache/wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:40:00.041 +13:59:48.07
Second-epoch image center 10:40:00.997 +13:59:57.71
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:40:00.041 +13:59:48.07
Second-epoch image center 10:40:04.047 +13:59:16.23
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:40:00.997 +13:59:57.71
Second-epoch second image center 10:40:04.047 +13:59:16.23
Angular distance between the image centers 0.01688 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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits &> /tmp/tmp.5EPwPWrdCv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits &> /tmp/tmp.ilZCYf0czm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits &> /tmp/tmp.31qOqjrh8N
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits &> /tmp/tmp.YX10ShmsX5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits and wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits and wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
Found non-empty wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits and wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
The reference image (wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits) and catalog (wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat) found
'wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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 3596 out of 6443 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.884590
a=0.000000 b=1.000000 c=22.884590
From vast_summary.log: estimated ref. image limiting mag.: -7.53
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
____ 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:
2.0 pix Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
2.1 pix Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
2.1 pix fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
2.1 pix fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
Limiting magnitude estimates:
15.4 mag. Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
15.4 mag. Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
15.3 mag. fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
15.3 mag. fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
All-image limiting magnitude estimate: 15.3 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5EPwPWrdCv (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits' -> 'wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
WCS-calibrated image found: wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
Checking if the catalog wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat corresponding to the image wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat corresponding to the image wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
WCS catalog name: wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=439, passed=6443
Got 6443 stars (including 5991 good ones) from the SExtractor catalog wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
util/solve_plate_with_UCAC5 got 6443 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 875 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: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
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 875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 875 stars left (next iteration limit 962)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits -region wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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.ilZCYf0czm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.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-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits' -> 'wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
WCS-calibrated image found: wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
Checking if the catalog wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat corresponding to the image wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat corresponding to the image wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
WCS catalog name: wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=445, passed=6432
Got 6432 stars (including 5975 good ones) from the SExtractor catalog wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat
util/solve_plate_with_UCAC5 got 6432 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 871 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: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 871 stars left (next iteration limit 958)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits -region wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.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.31qOqjrh8N (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
WCS_IMAGE_NAME=wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
WCS-calibrated image found: wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
Checking if the catalog wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
WCS catalog name: wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=414, passed=6305
Got 6305 stars (including 5885 good ones) from the SExtractor catalog wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits.cat
util/solve_plate_with_UCAC5 got 6305 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 869 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: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
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 869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 869 stars left (next iteration limit 955)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits -region wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.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.YX10ShmsX5 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
WCS_IMAGE_NAME=wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
WCS-calibrated image found: wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
Checking if the catalog wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
WCS catalog name: wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=437, passed=6263
Got 6263 stars (including 5821 good ones) from the SExtractor catalog wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat
util/solve_plate_with_UCAC5 got 6263 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 869 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 869 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: 0.29"
Excluding outliers - 869 stars left (next iteration limit 955)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits -region wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits'
Saving fully-calibrated image wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits'
Preparing the HTML report for the field Leo-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20403.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 20363_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
Preparing report for the candidate 20363_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20368_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 20368_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 11:12:24.13 +18:45:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.69, MAG_FAINT_SEARCH_LIMIT=11.67)GAIADR2_OUTPUT=# 1.865 3972032690743422080 168.10012059388 +18.75650268387 10.3955 9.7582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20389_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
Preparing report for the candidate 20389_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20403_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
Preparing report for the candidate 20403_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20423_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 20423_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:22:13.63 +17:06:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.285 3890327157049937664 155.55686882537 +17.10122102910 12.2972 11.8101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:52:52.05 +10:53:02.3
10:22:53.94 +12:12:12.0
11:02:43.21 +10:15:46.0
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
SExtractor catalog cache: saved Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat to cache
SExtractor catalog cache: saved Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
Creating symlink local_wcs_cache/wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits exists and is non-empty
wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits exists and is non-empty
wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits exists and is non-empty
wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:40:00.041 +13:59:48.07
Second-epoch image center 10:40:00.997 +13:59:57.71
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:40:00.041 +13:59:48.07
Second-epoch image center 10:40:04.047 +13:59:16.23
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:40:00.997 +13:59:57.71
Second-epoch second image center 10:40:04.047 +13:59:16.23
Angular distance between the image centers 0.01688 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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits &> /tmp/tmp.K2Sz89WCp3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits &> /tmp/tmp.M8IcuTCv5z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits &> /tmp/tmp.WeXus8rRoe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits &> /tmp/tmp.bMiufq6yfz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits and wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits and wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
Found non-empty wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits and wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
The reference image (wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits) and catalog (wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat) found
'wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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 3641 out of 34456 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.780203
a=0.000000 b=1.000000 c=22.780203
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.49
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 39 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
1.9 pix Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
2.0 pix fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
2.0 pix fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
Limiting magnitude estimates:
15.5 mag. Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
15.5 mag. Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
15.5 mag. fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
15.5 mag. fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.K2Sz89WCp3 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits' -> 'wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
WCS-calibrated image found: wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
Checking if the catalog wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat corresponding to the image wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat corresponding to the image wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits
WCS catalog name: wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1356, passed=34443
Got 34443 stars (including 33015 good ones) from the SExtractor catalog wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat
util/solve_plate_with_UCAC5 got 34443 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 875 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: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 875 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: 0.26"
Excluding outliers - 875 stars left (next iteration limit 962)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits -region wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q1b1x1_2026-01-18_02-53-36_20.00sec_-15.00C_LIGHT_0402.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.M8IcuTCv5z (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.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-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits' -> 'wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
WCS_IMAGE_NAME=wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
WCS-calibrated image found: wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
Checking if the catalog wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat corresponding to the image wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits alredy exist and is non-empty...
Catalog wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat corresponding to the image wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits
WCS catalog name: wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1357, passed=34514
Got 34514 stars (including 33102 good ones) from the SExtractor catalog wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat
util/solve_plate_with_UCAC5 got 34514 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 878 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: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 878 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: 0.26"
Excluding outliers - 878 stars left (next iteration limit 965)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits -region wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-05-Q1b1x1_2026-01-18_02-54-16_20.00sec_-15.00C_LIGHT_0403.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.WeXus8rRoe (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
WCS_IMAGE_NAME=wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
WCS-calibrated image found: wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
Checking if the catalog wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits.cat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
WCS catalog name: wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1260, passed=33537
Got 33537 stars (including 32213 good ones) from the SExtractor catalog wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits.cat
util/solve_plate_with_UCAC5 got 33537 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 873 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: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 873 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: 0.26"
Excluding outliers - 873 stars left (next iteration limit 960)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits -region wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.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.bMiufq6yfz (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
WCS_IMAGE_NAME=wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
WCS-calibrated image found: wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
Checking if the catalog wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat corresponding to the image wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
WCS catalog name: wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1270, passed=34052
Got 34052 stars (including 32727 good ones) from the SExtractor catalog wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat
util/solve_plate_with_UCAC5 got 34052 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 870 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: 0.33"
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 870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 870 stars left (next iteration limit 957)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits -region wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/wcs_fd_Leo-05-Q1b1x1_2026-02-12_02-59-40_20.00sec_-14.90C_LIGHT_0420.fits
Saving fully-calibrated image wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-05-Q1b1x1_030144_TTUQ1b1x1_17879_KNbHSCij/wcs_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421.fits
Preparing the HTML report for the field Leo-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out50025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out50263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52312.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out22857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52766.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 62s
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: 7s
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Considering the candidate 52305_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52305_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 11:11:29.97 +15:35:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 0.677 3970283921794991872 167.87469630814 +15.59925753593 14.4663 14.0344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52306_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52306_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 11:06:07.79 +13:11:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 0.889 3967893652235737600 166.53268207832 +13.19671695549 14.3049 13.5942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52310_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52310_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:51:42.73 +18:46:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.269 3983373637788051456 162.92798299738 +18.77532792076 14.2611 13.8002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52311_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52311_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:09:01.97 +09:34:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52312_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52312_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:09:58.59 +09:42:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 0.956 3876864912773220864 152.49439425947 +09.70059905643 13.7186 13.0375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.956#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52313_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52313_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 11:03:55.71 +15:01:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.664 3969394073290691968 165.98180499784 +15.01798973554 13.4186 12.9513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52327_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52327_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:52:52.06 +10:53:02.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52333_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52333_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 11:12:24.11 +18:45:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.62, MAG_FAINT_SEARCH_LIMIT=11.60)GAIADR2_OUTPUT=# 1.519 3972032690743422080 168.10012059388 +18.75650268387 10.3955 9.7582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52352_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52352_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:22:53.94 +12:12:12.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52366_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52366_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 11:02:43.21 +10:15:46.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52372_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52372_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:57:36.29 +15:44:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.444 3981370606775478656 164.40112877926 +15.74784762691 12.0685 11.4172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52393_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
Preparing report for the candidate 52393_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
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Considering the candidate 52415_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
Preparing report for the candidate 52415_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
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Considering the candidate 52419_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
Preparing report for the candidate 52419_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
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Considering the candidate 52432_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52432_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:25:10.99 +09:35:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 0.712 3876142735496843904 156.29586271742 +09.59725955327 13.1147 12.4778 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52478_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52478_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:08:54.85 +08:51:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.509 3875248527601215488 152.22840176661 +08.85539033531 13.3228 12.7807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52500_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52500_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 52543_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52543_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:28:21.55 +15:46:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 0.379 3889202498388997504 157.08989966422 +15.77112224751 13.5667 13.1009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52557_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
Preparing report for the candidate 52557_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
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Considering the candidate 52572_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
Preparing report for the candidate 52572_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
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Considering the candidate 52607_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
Preparing report for the candidate 52607_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
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Considering the candidate 52608_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52608_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:56:59.71 +15:30:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 0.525 3981360466357129984 164.24869115204 +15.50383553244 13.8873 13.3586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52611_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52611_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:43:14.34 +15:04:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 0.246 3886092495389812608 160.80970369312 +15.08113507200 13.9259 13.2857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52616_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52616_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:42:06.39 +09:22:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.473 3869136101944504704 160.52631607480 +09.36883793585 14.0166 13.4840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52620_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
Preparing report for the candidate 52620_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
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Considering the candidate 52649_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
Preparing report for the candidate 52649_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
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Considering the candidate 52682_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
Preparing report for the candidate 52682_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
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Considering the candidate 52702_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52702_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 11:07:54.73 +17:43:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 0.713 3971570075521463424 166.97783631441 +17.71763640591 14.3461 13.7897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52710_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
Preparing report for the candidate 52710_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
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Considering the candidate 52723_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52723_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 11:12:20.67 +18:25:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.399 3972006203680426112 168.08584229451 +18.43124644804 14.2354 13.6466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52724_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52724_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:31:36.83 +10:12:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 0.889 3882152807788897920 157.90357495901 +10.21636472685 14.2611 13.6845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52726_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52726_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:43:26.89 +09:52:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 0.943 3869563227852340608 160.86198975054 +09.88178467738 14.4417 13.7901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52742_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52742_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:56:27.71 +16:02:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 1.739 3981440288324861312 164.11514577276 +16.04159389838 14.5966 14.0585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52751_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52751_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 10:14:59.43 +12:33:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 4.564 3880881703627625472 153.74645020311 +12.56523521677 14.5289 14.0504 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52752_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 52752_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 11:08:23.83 +11:22:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 0.653 3964377379690424832 167.09936076383 +11.37966518891 14.3828 13.8707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52766_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
Preparing report for the candidate 52766_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
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Considering the candidate 50263_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 50263_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
**** FOUND 11:11:08.34 +18:04:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 0.457 3971967720773464576 167.78483861678 +18.08223402335 12.9057 12.4450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 50025_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421
The candidate 50025_fd_Leo-05-Q1b1x1_2026-02-12_03-00-32_20.00sec_-15.00C_LIGHT_0421 did not pass the final checks
