This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy
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 12.3661* 11 02 04.51 +24 43 18.5 10.5 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,2461083.8661,10.46,0.05,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 20260212.3661 10.46CV 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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:02:04.51 +24:43:18.5 ;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-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_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 12.3661* 11 18 36.43 +25 24 47.6 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
VARIABLE_NAME,2461083.8661,11.88,0.05,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 20260212.3661 11.88CV 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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:18:36.43 +25:24:47.6 ;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-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_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 12.3661* 11 21 41.77 +20 09 57.9 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
target,2461083.8661,14.32,0.05,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
target 20260212.3661 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:21:41.77 +20:09:57.9 ;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-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_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 12.3661* 10 53 35.77 +18 05 30.0 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,2461083.8661,12.82,0.05,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
VARIABLE_NAME 20260212.3661 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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:53:35.77 +18:05:30.0 ;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-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_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 12.3661* 11 12 08.47 +24 31 18.7 13.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.8661,13.04,0.05,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 20260212.3661 13.04CV 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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:12:08.47 +24:31:18.7 ;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-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_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 12.3661* 10 51 38.76 +20 51 37.2 13.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.8661,13.54,0.05,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 20260212.3661 13.54CV 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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:51:38.76 +20:51:37.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_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 12.3661* 10 34 20.13 +17 06 35.0 13.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.8661,13.62,0.05,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 20260212.3661 13.62CV 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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:34:20.13 +17:06:35.0 ;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-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_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 12.3661* 11 34 34.36 +26 17 56.4 14.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.8661,14.26,0.05,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 20260212.3661 14.26CV 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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:34:34.36 +26:17:56.4 ;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-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20_00sec_-14_90C_LIGHT_0407_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20_00sec_-15_00C_LIGHT_0406_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: 2461082.86515985 11.02.2026 08:45:39.811 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
First image: 2461082.86515985 11.02.2026 08:45:39.811 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
Last image: 2461083.86646821 12.02.2026 08:47:32.853 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
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: 2 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): 6024
Objects passed selection criteria: 6024
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 5886.5
Average stars matched: 5767.75 (97.9827 %)
Memory usage VmPeak: 112180 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 02:49:39 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: 2461082.86515985 11.02.2026 08:45:39.811 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
First image: 2461082.86515985 11.02.2026 08:45:39.811 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
Last image: 2461083.86646821 12.02.2026 08:47:32.853 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 54
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 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): 31843
Objects passed selection criteria: 31762
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 31041.5
Average stars matched: 30013.8 (96.6891 %)
Memory usage VmPeak: 133620 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 02:50:47 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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
SExtractor catalog cache: saved Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat to cache
SExtractor catalog cache: saved Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.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: 2461083.86571984
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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits exists and is non-empty
Saving wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits to local_wcs_cache/
'wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits' -> 'local_wcs_cache/wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits'
wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits exists and is non-empty
Saving wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits to local_wcs_cache/
'wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits' -> 'local_wcs_cache/wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits'
wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits exists and is non-empty
Saving wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits to local_wcs_cache/
'wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits' -> 'local_wcs_cache/wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits'
wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits exists and is non-empty
Saving wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits to local_wcs_cache/
'wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits' -> 'local_wcs_cache/wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:04:36.437 +21:59:53.37
Second-epoch image center 11:04:37.598 +21:59:44.79
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:04:36.437 +21:59:53.37
Second-epoch image center 11:04:35.573 +22:00:06.06
Angular distance between the image centers 0.00 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:04:37.598 +21:59:44.79
Second-epoch second image center 11:04:35.573 +22:00:06.06
Angular distance between the image centers 0.00980 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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits &> /tmp/tmp.CP7UEZIK8I
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits &> /tmp/tmp.KC0aGEJaIx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits &> /tmp/tmp.sM1Ga9aGLx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits &> /tmp/tmp.BQ1Ff0C8ny
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits and wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits and wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat
Found non-empty wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits and wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat
The reference image (wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits) and catalog (wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat) found
'wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.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 3296 out of 5979 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.905169
a=0.000000 b=1.000000 c=22.905169
From vast_summary.log: estimated ref. image limiting mag.: -7.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
2.2 pix Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
2.1 pix fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
2.1 pix fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
Limiting magnitude estimates:
15.4 mag. Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
15.4 mag. Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
15.4 mag. fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
15.4 mag. fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 12.3 (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.CP7UEZIK8I (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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits' -> 'wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
WCS-calibrated image found: wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
Checking if the catalog wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
WCS catalog name: wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=393, passed=5979
Got 5979 stars (including 5578 good ones) from the SExtractor catalog wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat
util/solve_plate_with_UCAC5 got 5979 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 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits -region wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.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.KC0aGEJaIx (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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.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-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits' -> 'wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
WCS-calibrated image found: wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
Checking if the catalog wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
WCS catalog name: wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=398, passed=5893
Got 5893 stars (including 5486 good ones) from the SExtractor catalog wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat
util/solve_plate_with_UCAC5 got 5893 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 949 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: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits -region wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.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.sM1Ga9aGLx (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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
Checking if the catalog wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
WCS catalog name: wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=366, passed=5939
Got 5939 stars (including 5563 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits.cat
util/solve_plate_with_UCAC5 got 5939 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 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.26"
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 946 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits -region wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.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.BQ1Ff0C8ny (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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
Checking if the catalog wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
WCS catalog name: wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=382, passed=5876
Got 5876 stars (including 5486 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits.cat
util/solve_plate_with_UCAC5 got 5876 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 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits -region wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.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-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits'
Saving fully-calibrated image wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits'
Preparing the HTML report for the field Leo-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20195.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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 20193_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
The candidate 20193_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407 did not pass the final checks
**** FOUND 11:20:43.87 +22:52:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.15, MAG_FAINT_SEARCH_LIMIT=11.13)GAIADR2_OUTPUT=# 0.694 3991286754253836160 170.18295812116 +22.87471672612 10.1814 9.5966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20194_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
Preparing report for the candidate 20194_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20195_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
Preparing report for the candidate 20195_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20196_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
The candidate 20196_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407 did not pass the final checks
**** FOUND 11:08:38.69 +19:58:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.038 3984498305039862912 167.16121795707 +19.97958895646 12.3258 11.8758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.038#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: 8s
Prepared the HTML report for the field Leo-03-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 ####
11:02:04.51 +24:43:18.5
11:18:36.43 +25:24:47.6
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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
SExtractor catalog cache: saved Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat to cache
SExtractor catalog cache: saved Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
Creating symlink local_wcs_cache/wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits exists and is non-empty
wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits exists and is non-empty
wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits exists and is non-empty
wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:04:36.437 +21:59:53.37
Second-epoch image center 11:04:37.598 +21:59:44.79
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:04:36.437 +21:59:53.37
Second-epoch image center 11:04:35.573 +22:00:06.06
Angular distance between the image centers 0.00 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:04:37.598 +21:59:44.79
Second-epoch second image center 11:04:35.573 +22:00:06.06
Angular distance between the image centers 0.00980 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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits &> /tmp/tmp.U6qFq6oPKr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits &> /tmp/tmp.NQm8qaYk04
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits &> /tmp/tmp.gj14PZGMf3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits &> /tmp/tmp.ry8vLirPI6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits and wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits and wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat
Found non-empty wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits and wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat
The reference image (wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits) and catalog (wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat) found
'wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.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 3329 out of 31291 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.798316
a=0.000000 b=1.000000 c=22.798316
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.53
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 17 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
2.0 pix Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
2.0 pix fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
2.0 pix fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
Limiting magnitude estimates:
15.5 mag. Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
15.5 mag. Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
15.5 mag. fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
15.5 mag. fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.8 (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.U6qFq6oPKr (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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.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-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits' -> 'wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
WCS-calibrated image found: wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
Checking if the catalog wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
WCS catalog name: wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1166, passed=31271
Got 31271 stars (including 30054 good ones) from the SExtractor catalog wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat
util/solve_plate_with_UCAC5 got 31271 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 943 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits -region wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q1b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.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.NQm8qaYk04 (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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.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-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits' -> 'wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
WCS-calibrated image found: wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
Checking if the catalog wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
WCS catalog name: wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=1184, passed=31263
Got 31263 stars (including 30025 good ones) from the SExtractor catalog wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat
util/solve_plate_with_UCAC5 got 31263 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 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits -region wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q1b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.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.gj14PZGMf3 (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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
Checking if the catalog wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
WCS catalog name: wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1140, passed=31216
Got 31216 stars (including 30018 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits.cat
util/solve_plate_with_UCAC5 got 31216 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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
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 945 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 - 945 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits -region wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.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.ry8vLirPI6 (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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
Checking if the catalog wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
WCS catalog name: wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1126, passed=31241
Got 31241 stars (including 30072 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits.cat
util/solve_plate_with_UCAC5 got 31241 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 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Leo-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits -region wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.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-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-46-28_20.00sec_-15.00C_LIGHT_0406.fits
Saving fully-calibrated image wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.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-03-Q1b1x1_024813_TTUQ1b1x1_31393_7UUlkkhy/wcs_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407.fits
Preparing the HTML report for the field Leo-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51988.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out51987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52058.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 51987_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
Preparing report for the candidate 51987_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
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Considering the candidate 51988_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
The candidate 51988_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407 did not pass the final checks
**** FOUND 11:07:32.63 +20:53:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.047 3985330669701917184 166.88596183351 +20.88706862501 13.7483 13.2800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51989_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
The candidate 51989_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407 did not pass the final checks
**** FOUND 11:10:28.72 +20:09:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 0.780 3984476108648859264 167.61968812333 +20.15813230667 13.3464 12.6897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51990_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
The candidate 51990_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407 did not pass the final checks
**** FOUND 11:02:04.51 +24:43:18.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 51991_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
The candidate 51991_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407 did not pass the final checks
**** FOUND 11:14:01.90 +20:34:39.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 51993_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
The candidate 51993_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407 did not pass the final checks
**** FOUND 11:18:36.43 +25:24:47.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 51999_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
Preparing report for the candidate 51999_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
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Considering the candidate 52003_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
Preparing report for the candidate 52003_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
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Considering the candidate 52007_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
The candidate 52007_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407 did not pass the final checks
**** FOUND 10:59:50.77 +25:18:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.851 3996291082643947776 164.96207182903 +25.30501913331 12.4601 11.3626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52012_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
The candidate 52012_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407 did not pass the final checks
**** FOUND 11:04:40.14 +24:19:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.617 3995233627335523072 166.16707137481 +24.33277986491 13.4023 12.9358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52020_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
Preparing report for the candidate 52020_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52024_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
Preparing report for the candidate 52024_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52044_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
The candidate 52044_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407 did not pass the final checks
**** FOUND 10:41:57.49 +22:29:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.747 722845194940141568 160.48931897669 +22.48474971871 14.0577 13.5140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52052_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
The candidate 52052_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407 did not pass the final checks
**** FOUND 10:43:05.56 +21:43:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 2.331 3989367767161200384 160.77271566068 +21.71653397415 14.4101 13.7633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52058_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
Preparing report for the candidate 52058_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
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Considering the candidate 52060_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
The candidate 52060_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407 did not pass the final checks
**** FOUND 10:53:01.78 +26:20:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 0.810 730021952148043904 163.25718012036 +26.34693624026 14.4807 13.9561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52062_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407
The candidate 52062_fd_Leo-03-Q1b1x1_2026-02-12_02-47-32_20.00sec_-14.90C_LIGHT_0407 did not pass the final checks