This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt
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!
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,2461098.8521,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.3521 10.56CV 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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:50:59.71 +26:52:46.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_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!
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,2461098.8521,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.3521 11.70CV 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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:05:53.65 +27:01:38.0 ;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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_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!
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,2461098.8521,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.3521 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:00:10.63 +25:38:05.6 ;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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_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 27.3521* 10 38 13.58 +19 09 18.5 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,2461098.8521,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.3521 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:38:13.58 +19:09:18.5 ;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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_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 27.3521* 10 40 23.76 +21 28 56.5 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,2461098.8521,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.3521 13.49CV 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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:40:23.76 +21:28:56.5 ;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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3521 2461098.8521 13.81 10:32:21.55 +26:14:16.5
206.51953 59.01984 galactic Leo Second-epoch detections are separated by 1.9" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 727597799591505920 | 10:32:22.00 +26:14:17.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3521* 10 32 21.55 +26 14 16.5 13.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 727597799591505920,2461098.8521,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 727597799591505920 20260227.3521 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:32:21.55 +26:14:16.5 ;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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3521 2461098.8521 14.01 10:38:46.57 +26:53:25.7
205.67836 60.53824 galactic LMi Second-epoch detections are separated by 2.7" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:38:46.57 +26:53:25.7 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461098.8521,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260227.3521 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:38:46.57 +26:53:25.7 ;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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 27.3521 2461098.8521 13.55 10:56:09.83 +19:23:58.9
223.05931 62.49247 galactic Leo Second-epoch detections are separated by 1.4" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J164.0409+19.3997 | 10:56:09.83 +19:23:58.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.381+/-0.036 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.3521* 10 56 09.83 +19 23 58.9 13.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J164.0409+19.3997,2461098.8521,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J164.0409+19.3997 20260227.3521 13.55CV 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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:56:09.83 +19:23:58.9 ;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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_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-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20_00sec_-15_00C_LIGHT_0113_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png resample_wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20_00sec_-15_00C_LIGHT_0112_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
Last image: 2461098.85237816 27.02.2026 08:27:15.473 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 20
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: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5781
Objects passed selection criteria: 5776
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 5212.5
Average stars matched: 5147 (98.7434 %)
Memory usage VmPeak: 112056 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 Fri Feb 27 04:49:25 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-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
Last image: 2461098.85237816 27.02.2026 08:27:15.473 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 64
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: 13 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): 29383
Objects passed selection criteria: 29309
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 27043.5
Average stars matched: 25903.5 (95.7846 %)
Memory usage VmPeak: 133516 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 Fri Feb 27 04:50:34 CST 2026
Host name: tau
############################################################
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst
CAMERA_SETTINGS= TTUQ2b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR=
EXCLUSION_LIST= ../exclusion_list_TTUQ2.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE=
FRAME_EDGE_OFFSET_PIX= 100
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
SExtractor catalog cache: enabled, directory /data_ssd/NMW-TexasTech/vast_sextractor_cache
Reference image directory is set to /data_ssd/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.cds.unistra.fr
GAIA_DR2_CLIENT=vizquery (lib/vizquery -> VizieR vizier.cds.unistra.fr)
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Leo-03-Q2b1x1
#######################################
########### Starting Leo-03-Q2b1x1 ###########
Processing Leo-03-Q2b1x1
server tau has sufficient free disk space available: 685887 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 685887 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.png' -> 'transient_report/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits_preview.png'
Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
renamed 'Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.png' -> 'transient_report/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits_preview.png'
Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 500.7820
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 455.5506
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1723.9252
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 557.0067
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1723.5784
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 557.9226
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 3.44247
INFO: SECOND_EPOCH__SD_ratio= 0.002
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR= FLAT_FIELD_FILE=
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
SExtractor catalog cache: saved Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat to cache
SExtractor catalog cache: saved Leo-03-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.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: 2461098.85178201
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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits exists and is non-empty
Saving wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits to local_wcs_cache/
'wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits' -> 'local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits'
wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits exists and is non-empty
Saving wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits to local_wcs_cache/
'wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits' -> 'local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits'
wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits exists and is non-empty
Saving wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits to local_wcs_cache/
'wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits' -> 'local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits'
wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits exists and is non-empty
Saving wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits to local_wcs_cache/
'wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits' -> 'local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.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 11:04:51.631 +21:58:13.07
Angular distance between the image centers 0.06 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 11:04:49.214 +21:57:28.85
Angular distance between the image centers 0.06 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 11:04:51.631 +21:58:13.07
Second-epoch second image center 11:04:49.214 +21:57:28.85
Angular distance between the image centers 0.01543 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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits &> /tmp/tmp.tItWTPfIIu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_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-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits &> /tmp/tmp.3Rro2nI8Vd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_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_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits &> /tmp/tmp.LgA6nwcYbm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits &> /tmp/tmp.jAlPmAKxZ7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-03-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits and wcs_Leo-03-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits and wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat
Found non-empty wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits and wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat
The reference image (wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits) and catalog (wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat) found
'wcs_Leo-03-Q2b1x1_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 20 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
2.2 pix Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
2.5 pix Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
2.4 pix Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
Limiting magnitude estimates:
15.4 mag. Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
15.4 mag. Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
14.8 mag. Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
14.8 mag. Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 12.1 (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.tItWTPfIIu (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits' -> 'wcs_Leo-03-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits -region wcs_Leo-03-Q2b1x1_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-Q2b1x1_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.3Rro2nI8Vd (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits' -> 'wcs_Leo-03-Q2b1x1_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-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits -region wcs_Leo-03-Q2b1x1_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-Q2b1x1_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.LgA6nwcYbm (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_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.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_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=350, passed=4561
Got 4561 stars (including 4207 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits.cat
util/solve_plate_with_UCAC5 got 4561 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
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 946 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: 0.27"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits -region wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.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.jAlPmAKxZ7 (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_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.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_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=377, passed=4538
Got 4538 stars (including 4156 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits.cat
util/solve_plate_with_UCAC5 got 4538 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.30"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits -region wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.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
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Leo-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20209.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out20210.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out20195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20200.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 20194_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20194_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:20:43.91 +22:52:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.40, MAG_FAINT_SEARCH_LIMIT=11.38)GAIADR2_OUTPUT=# 0.480 3991286754253836160 170.18295812116 +22.87471672612 10.1814 9.5966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20195_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
Preparing report for the candidate 20195_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
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Considering the candidate 20199_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20199_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:56:23.21 +22:21:28.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20200_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
Preparing report for the candidate 20200_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
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Considering the candidate 20201_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20201_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:08:45.79 +22:33:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.216 3991816791872894848 167.19075113037 +22.56135258794 12.3247 11.8575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20202_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20202_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:05:21.65 +21:47:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.436 3991667975551227776 166.34032245220 +21.79075319647 12.3166 11.8405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20204_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20204_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:09:50.11 +22:03:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.251 3991550057223972224 167.45875298558 +22.05169857485 12.3555 11.8755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20205_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20205_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:06:41.64 +22:58:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.161 3994847969336931072 166.67353670087 +22.97766832138 12.4798 12.3661 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20207_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20207_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:08:38.68 +19:58:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.175 3984498305039862912 167.16121795707 +19.97958895646 12.3258 11.8758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20209_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20209_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:09:03.18 +22:47:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.326 3991847539543379968 167.26316003004 +22.78467494677 12.4787 12.1079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20210_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20210_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:05:41.95 +22:36:41.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)
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Considering the candidate 20212_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20212_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:07:55.98 +23:45:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.399 3995328150976100224 166.98332322559 +23.76461619034 12.3893 11.8751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20213_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20213_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:08:37.16 +22:17:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.298 3991756696690530816 167.15491967920 +22.28563246461 12.5048 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20215_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20215_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:03:03.52 +22:53:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.503 3994816465752179968 165.76458918147 +22.88967557383 12.2301 11.3268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20216_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20216_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:14:13.40 +24:16:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.125 3992425504702837632 168.55581191210 +24.26911030209 12.3782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20217_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20217_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:00:24.74 +20:15:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.066 3985409795884124160 165.10310221177 +20.26189391692 12.3990 11.7388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20222_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20222_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:56:19.82 +23:48:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.495 3995894807485884800 164.08263844231 +23.80489988509 12.4371 11.7682 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20225_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20225_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:02:31.24 +23:45:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.240 3995186520134248448 165.63023612475 +23.75772950218 12.5717 12.1674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20226_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20226_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:14:35.15 +24:28:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.150 3992438011647601280 168.64641289723 +24.47017242930 12.4120 11.9648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20228_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 20228_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:16:32.66 +23:15:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.164 3992096853805044352 169.13611960311 +23.25552443473 12.5400 12.0993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Leo-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:50:59.71 +26:52:46.1
11:05:53.65 +27:01:38.0
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
SExtractor catalog cache: saved Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat to cache
SExtractor catalog cache: saved Leo-03-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
Creating symlink local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
Creating symlink local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
Creating symlink local_wcs_cache/wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits exists and is non-empty
wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits exists and is non-empty
wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits exists and is non-empty
wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.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 11:04:51.631 +21:58:13.07
Angular distance between the image centers 0.06 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 11:04:49.214 +21:57:28.85
Angular distance between the image centers 0.06 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 11:04:51.631 +21:58:13.07
Second-epoch second image center 11:04:49.214 +21:57:28.85
Angular distance between the image centers 0.01543 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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits &> /tmp/tmp.eHBE8NuEPu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_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-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits &> /tmp/tmp.roPdiN0NKO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_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_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits &> /tmp/tmp.OrTX27Y00S
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits &> /tmp/tmp.pp7csvAtli
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-03-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits and wcs_Leo-03-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits and wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat
Found non-empty wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits and wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat
The reference image (wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits) and catalog (wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat) found
'wcs_Leo-03-Q2b1x1_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 39 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
2.0 pix Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
2.5 pix Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
2.4 pix Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
Limiting magnitude estimates:
15.5 mag. Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
15.5 mag. Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
14.9 mag. Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
15.0 mag. Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.3 (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.eHBE8NuEPu (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits' -> 'wcs_Leo-03-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-45-39_20.00sec_-15.00C_LIGHT_0391.fits -region wcs_Leo-03-Q2b1x1_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-Q2b1x1_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.roPdiN0NKO (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits' -> 'wcs_Leo-03-Q2b1x1_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-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-11_02-46-15_20.00sec_-15.00C_LIGHT_0392.fits -region wcs_Leo-03-Q2b1x1_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-Q2b1x1_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.OrTX27Y00S (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_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.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_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=928, passed=23032
Got 23032 stars (including 22076 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits.cat
util/solve_plate_with_UCAC5 got 23032 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.28"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits -region wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-02-27_02-26-23_20.00sec_-15.00C_LIGHT_0112.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.pp7csvAtli (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_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.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_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
WCS-calibrated image found: wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
Checking if the catalog wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits.cat corresponding to the image wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits
WCS catalog name: wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=995, passed=23400
Got 23400 stars (including 22375 good ones) from the SExtractor catalog wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits.cat
util/solve_plate_with_UCAC5 got 23400 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 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: 0.30"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-03-Q2b1x1_044707_TTUQ2b1x1_24795_40Fp6zZt/Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits -region wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113.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
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Leo-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52069.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52312.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out28108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52457.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 51987_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:34:00.83 +23:40:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 1.104 722523145408042624 158.50364806744 +23.67578038974 13.6754 13.2152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51990_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 51990_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:36:31.18 +18:51:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.031 3986868096194683648 159.13030119829 +18.86034794565 13.8268 13.3819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51996_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 51996_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:34:21.64 +24:21:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 4.801 724270922219375104 158.59160605763 +24.35935497495 13.2956 12.7770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51997_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 51997_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:32:52.75 +22:36:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.284 721560591697068288 158.22003896154 +22.61103153011 13.7385 13.2686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51999_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 51999_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:31:52.08 +24:57:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 4.780 724363521714257024 157.96845840189 +24.95073075000 12.8765 12.3731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52001_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52001_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:31:46.33 +24:50:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 4.167 724336137002779392 157.94177493437 +24.84571923125 12.8708 12.2520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52006_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52006_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 52007_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52007_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:42:18.25 +26:56:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 5.874 725055870442247552 160.57421211100 +26.93990904849 12.9360 12.4251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.874#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52008_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52008_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:36:31.88 +26:13:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.340 727905632783099904 159.13354313914 +26.23015917711 12.5664 11.9719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.340#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52009_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52009_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 52013_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52013_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:34:36.57 +18:19:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.998 3974252677734972416 173.65295946842 +18.32284566217 13.4796 13.3094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52017_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52017_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:10:28.77 +20:09:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.080 3984476108648859264 167.61968812333 +20.15813230667 13.3464 12.6897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52018_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52018_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:31:31.46 +25:07:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 2.472 727370131964955776 157.88173144463 +25.12257887415 9.9893 9.3761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52022_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52022_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:50:59.71 +26:52:46.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52023_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52023_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:14:01.90 +20:34:39.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 52058_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52058_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:05:53.65 +27:01:38.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52069_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52069_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:08:25.04 +21:02:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.706 3991337988918958464 167.10449460447 +21.04976482179 12.4709 11.9671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52119_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52119_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:55:27.53 +24:43:54.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)
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Considering the candidate 52165_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
Preparing report for the candidate 52165_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
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Considering the candidate 52175_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
Preparing report for the candidate 52175_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
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Considering the candidate 52192_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52192_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:08:42.10 +24:38:46.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52300_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52300_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:13:34.12 +20:06:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.317 3990286026873829504 168.39242382339 +20.11514183302 13.2007 12.2296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52305_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52305_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:29:39.07 +26:34:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52312_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52312_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:10:59.33 +18:22:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.879 3971993868534382464 167.74746520623 +18.37612653702 13.5604 13.0216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52319_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
Preparing report for the candidate 52319_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
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Considering the candidate 52351_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52351_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:10:51.48 +21:58:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.023 3991534728485276800 167.71459070806 +21.98281198820 14.0392 13.5749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52358_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
Preparing report for the candidate 52358_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
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Considering the candidate 52365_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52365_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:46:35.69 +24:40:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.289 723720238692754560 161.64903890106 +24.67247244754 13.7628 13.0410 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52393_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52393_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:25:50.72 +26:45:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52394_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52394_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:21:02.58 +23:49:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.643 3993597244795692928 170.26091260952 +23.82340105572 13.9655 13.4913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52398_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52398_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:34:40.78 +23:20:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.500 3981006148735077760 173.67037047393 +23.33420010007 13.1435 12.1783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52433_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52433_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:00:33.52 +23:43:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.896 3995104812676549888 165.13899362298 +23.71862809731 14.5362 14.1211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52457_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
Preparing report for the candidate 52457_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
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Considering the candidate 52484_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52484_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:18:34.84 +25:32:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.479 3997095134881031808 169.64545909030 +25.53660188348 14.1151 13.6242 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52524_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52524_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 11:35:06.41 +20:25:20.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52547_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52547_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:30:59.16 +26:09:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 3.379 727575195179050240 157.74688330374 +26.15240101821 12.8121 12.1806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52599_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52599_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:35:16.85 +26:29:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 4.209 727926935820875264 158.82151092503 +26.48653304587 13.2170 12.7516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52682_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113
The candidate 52682_Leo-03-Q2b1x1_2026-02-27_02-27-15_20.00sec_-15.00C_LIGHT_0113 did not pass the final checks