This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.2390* 10 07 43.43 +23 59 30.4 10.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RR Leo,2461098.7390,10.23,0.05,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
RR Leo 20260227.2390 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:07:43.43 +23:59:30.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_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 27.2390* 10 38 21.11 +19 08 54.5 13.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7390,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.2390 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:38:21.11 +19:08:54.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_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 27.2390* 10 21 31.06 +18 36 18.7 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,2461098.7390,13.47,0.05,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 20260227.2390 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:21:31.06 +18:36:18.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_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 27.2390* 10 01 27.30 +23 43 23.5 13.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7390,13.22,0.05,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 20260227.2390 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:01:27.30 +23:43:23.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_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 27.2390* 10 08 47.52 +19 32 48.4 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,2461098.7390,13.54,0.05,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 20260227.2390 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:08:47.52 +19:32:48.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_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 27.2390* 10 40 29.18 +21 28 44.4 13.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7390,13.60,0.05,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 20260227.2390 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:40:29.18 +21:28:44.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_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 27.2390* 09 36 44.70 +18 35 25.2 13.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7390,13.60,0.05,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 20260227.2390 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:36:44.70 +18:35:25.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_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 27.2390* 10 09 40.00 +18 45 42.9 13.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7390,13.80,0.05,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 20260227.2390 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:09:40.00 +18:45:42.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_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 27.2390* 09 37 04.27 +24 36 23.9 13.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7390,13.84,0.05,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 20260227.2390 13.84CV 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-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:37:04.27 +24:36:23.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_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 27.2390* 09 59 59.35 +22 38 03.2 14.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7390,14.04,0.05,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 20260227.2390 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:59:59.35 +22:38:03.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_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 27.2390* 09 55 18.29 +17 58 53.1 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.7390,14.45,0.05,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 20260227.2390 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:55:18.29 +17:58:53.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20_00sec_-15_00C_LIGHT_0255_fits__*pix.png resample_wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.75562678 09.01.2026 06:07:56.154 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
First image: 2461049.75562678 09.01.2026 06:07:56.154 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Last image: 2461098.73928893 27.02.2026 05:44:24.564 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 52
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.80
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5273
Objects passed selection criteria: 5272
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 4823.5
Average stars matched: 4690.25 (97.2375 %)
Memory usage VmPeak: 111560 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 04:49:09 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.75562678 09.01.2026 06:07:56.154 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
First image: 2461049.75562678 09.01.2026 06:07:56.154 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Last image: 2461098.73928893 27.02.2026 05:44:24.564 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 56
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 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): 30048
Objects passed selection criteria: 29986
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: 27959.5
Average stars matched: 26623 (95.2199 %)
Memory usage VmPeak: 132628 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 04:50:16 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-02-Q2b1x1
#######################################
########### Starting Leo-02-Q2b1x1 ###########
Processing Leo-02-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-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.png' -> 'transient_report/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits_preview.png'
Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
renamed 'Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.png' -> 'transient_report/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits_preview.png'
Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.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= 913.1746
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 506.8818
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1972.5054
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 630.3413
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1970.5288
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 615.3755
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.16005
INFO: SECOND_EPOCH__SD_ratio= 0.024
----------------------------------------------
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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.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-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.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: 2461098.73875226
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits exists and is non-empty
Saving wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits to local_wcs_cache/
'wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits' -> 'local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits'
wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits exists and is non-empty
Saving wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits to local_wcs_cache/
'wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits' -> 'local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits'
wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits exists and is non-empty
Saving wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits to local_wcs_cache/
'wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits' -> 'local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits'
wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits exists and is non-empty
Saving wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits to local_wcs_cache/
'wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits' -> 'local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:14.676 +22:00:04.67
Second-epoch image center 10:09:05.783 +22:01:54.42
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:09:14.676 +22:00:04.67
Second-epoch image center 10:09:07.955 +22:02:00.24
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:09:05.783 +22:01:54.42
Second-epoch second image center 10:09:07.955 +22:02:00.24
Angular distance between the image centers 0.00854 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits &> /tmp/tmp.NnIKwECfVO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits &> /tmp/tmp.qHOZrxcIwv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits &> /tmp/tmp.909B20D3x1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits &> /tmp/tmp.Tf5i56shRV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
Found non-empty wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
The reference image (wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits) and catalog (wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat) found
'wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 3674 out of 5334 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.866726
a=0.000000 b=1.000000 c=22.866726
From vast_summary.log: estimated ref. image limiting mag.: -7.80
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.07
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 52 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
2.1 pix Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
2.4 pix Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
2.4 pix Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
Limiting magnitude estimates:
15.1 mag. Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
15.1 mag. Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
14.5 mag. Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
14.5 mag. Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.8 (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.NnIKwECfVO (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-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits' -> 'wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=391, passed=5334
Got 5334 stars (including 4935 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
util/solve_plate_with_UCAC5 got 5334 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 907 stars left (next iteration limit 997)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits -region wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qHOZrxcIwv (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-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.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-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits' -> 'wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=401, passed=5315
Got 5315 stars (including 4910 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat
util/solve_plate_with_UCAC5 got 5315 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 910 stars left (next iteration limit 1001)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits -region wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.909B20D3x1 (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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=566, passed=4457
Got 4457 stars (including 3889 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits.cat
util/solve_plate_with_UCAC5 got 4457 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 906 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: 0.36"
Excluding outliers - 906 stars left (next iteration limit 996)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits -region wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.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.Tf5i56shRV (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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=471, passed=4330
Got 4330 stars (including 3857 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits.cat
util/solve_plate_with_UCAC5 got 4330 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 913 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: 0.35"
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 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 912 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits -region wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.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-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20367.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20395.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20404.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out20414.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out03624.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20344_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20344_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:07:32.24 +22:06:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 0.205 629941891235056896 151.88439250053 +22.11007076182 12.5058 11.8501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20349_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20349_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:12:00.05 +19:22:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 0.480 625195333894472704 153.00031639484 +19.36666422949 12.2449 11.8459 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20356_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20356_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:05:14.01 +22:39:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 0.401 630033945265917184 151.30839814617 +22.65164067744 12.0702 11.6243 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20361_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20361_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:10:22.16 +21:04:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 0.142 628524861261652224 152.59229892386 +21.07600465745 12.1386 11.7487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20367_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20367_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:03:52.01 +22:07:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.294 629606097803887616 150.96666245314 +22.12670817482 12.0826 11.6201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20368_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20368_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:05:17.77 +21:32:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.500 629521740350884864 151.32414908971 +21.54195757459 12.0386 11.3669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20372_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20372_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:09:18.82 +22:26:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.117 629978419928722432 152.32840593581 +22.44083006318 12.1887 11.7455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20373_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20373_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:06:50.35 +22:26:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 0.260 629966080487764224 151.70980767003 +22.43473486885 12.1907 11.7733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20374_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20374_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:01:35.87 +22:08:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.065 629804864595039616 150.39946919491 +22.14729285904 12.0456 11.6355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20375_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20375_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:08:30.98 +22:54:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 0.381 630056068642429952 152.12908413443 +22.91067203717 12.1298 11.6271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20376_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20376_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:09:22.78 +20:09:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 0.251 628303893784383872 152.34484985134 +20.16422515109 12.1590 11.7143 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20378_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20378_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:12:57.31 +22:17:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 0.787 629245522414660608 153.23902701590 +22.29949292473 12.2211 11.7044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20379_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20379_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:03:44.36 +20:28:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 0.856 628557503013108608 150.93506036915 +20.47299521806 12.2524 11.9928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20380_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20380_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:13:21.84 +21:51:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 0.340 628950544060253696 153.34110154986 +21.86120093212 12.2369 11.7791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.340#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20381_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20381_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:08:38.93 +23:06:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 0.381 630156643891763840 152.16209457372 +23.10248869076 12.2057 11.7233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20382_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20382_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:13:40.81 +20:44:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 0.129 625811885039771648 153.42007130375 +20.73367191944 12.1638 11.5538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20383_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20383_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:13:30.73 +22:05:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 0.276 629050290380736640 153.37812058241 +22.08807866640 12.1696 11.6032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20384_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20384_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:06:00.17 +21:02:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.356 628603824235803904 151.50079797830 +21.03897501668 12.1531 11.4939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20386_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20386_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:09:17.94 +21:15:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 0.225 628713599304482944 152.32481293656 +21.26561699694 12.1123 11.4437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20387_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20387_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:08:04.85 +21:21:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 0.341 628732123498811392 152.02017268227 +21.36617206112 12.2412 11.7785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20389_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20389_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:09:28.00 +20:05:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 0.294 628301110645577728 152.36658060097 +20.08870690787 12.3533 12.2464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20390_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20390_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:05:42.59 +23:05:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.374 630262055273791744 151.42735817316 +23.08646448896 12.1257 11.5690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20393_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20393_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:06:05.97 +22:54:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 0.496 630044871662678528 151.52498430356 +22.90995497647 12.1183 11.4533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20394_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20394_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:04:07.89 +23:04:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.477 630247521104462464 151.03294213756 +23.07366069879 12.1500 11.6995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20395_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20395_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:14:27.62 +22:16:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.393 629060529582768512 153.61496543778 +22.27852335021 12.2745 11.8326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20396_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20396_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:12:57.83 +22:40:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.193 629319636369811328 153.24095802104 +22.67810920335 12.2285 11.7142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.193#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20397_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20397_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:01:11.24 +21:39:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.288 629503048653652992 150.29691571346 +21.66383825559 12.1391 11.7245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20398_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20398_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:09:07.89 +23:33:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.442 630185849669368960 152.28278654028 +23.55340776312 12.2660 11.8601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20399_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20399_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:01:18.67 +20:23:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.616 627110476991440512 150.32796402030 +20.38655454647 12.1738 11.7344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20400_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20400_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:16:01.91 +21:34:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.332 628962569968974336 154.00797873210 +21.57372916619 12.1631 11.5741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20401_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20401_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:09:25.04 +21:37:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.368 629115367725350784 152.35444036086 +21.61730141111 12.3574 11.9409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20402_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20402_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:07:58.06 +22:31:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.740 629970620268088576 151.99199025119 +22.52738926643 12.3297 11.9346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20403_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20403_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:07:29.22 +22:21:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.428 629967386157823360 151.87176876552 +22.36124358067 12.2990 11.7751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20404_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20404_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:01:51.54 +20:24:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.655 627099795408344576 150.46477309918 +20.40690291568 12.2856 11.9362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20405_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20405_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:18:11.24 +21:53:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.157 625997535001452928 154.54687254279 +21.88475389162 12.2709 11.7872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20407_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20407_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:05:53.85 +21:01:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.422 628650347321554816 151.47445593720 +21.01982704989 12.3638 11.8530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20408_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20408_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:10:39.21 +21:00:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.804 628511705777640192 152.66344947487 +21.00387903509 12.4565 11.8011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20410_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20410_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 09:59:04.52 +20:50:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.990 627937142232100480 149.76860257034 +20.83372620155 11.8206 10.8999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20411_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20411_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:09:19.86 +20:48:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.681 628478544334714368 152.33294640073 +20.80325993881 12.2473 11.5599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20414_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20414_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:02:37.97 +22:23:07.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20415_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20415_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:06:03.39 +23:46:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.343 630435541888294272 151.51415016324 +23.77218532898 12.1861 11.7228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20419_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20419_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:11:11.26 +22:12:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.339 629164059769651840 152.79701713371 +22.20109623902 12.3820 11.8954 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20420_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20420_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:15:45.30 +21:46:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.292 628983426330161024 153.93867441979 +21.77842941642 12.3494 11.8193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20421_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20421_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:09:29.38 +22:39:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.415 629990063584838272 152.37246682094 +22.65883893992 12.2989 11.7050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20423_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20423_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:09:19.97 +22:52:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.315 630006663633619072 152.33311663485 +22.88030034588 12.3633 11.8675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20425_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20425_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 09:59:21.06 +20:50:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.734 627937760707388032 149.83792552756 +20.84131553855 12.2508 11.8165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20426_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20426_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:01:46.58 +19:43:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.565 626993452018206976 150.44420538635 +19.71708761811 12.1756 11.5605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20428_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20428_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:03:31.92 +22:12:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.621 629619291943421696 150.88316646371 +22.20588283866 12.3020 11.7674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20429_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20429_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:03:55.27 +24:12:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.642 642485502133918976 150.98045902219 +24.21487996191 12.2594 11.9773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20430_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20430_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:13:15.64 +23:24:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.147 726206298906985856 153.31517536231 +23.40365447489 12.3651 11.9757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20431_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 20431_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:00:05.26 +19:27:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.268 626901020026622720 150.02199077747 +19.46535917469 12.1515 11.5482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03624_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 03624_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 15s
Prepared the HTML report for the field Leo-02-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 ####
10:07:43.43 +23:59:30.4
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Creating symlink local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Creating symlink local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
Creating symlink local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits exists and is non-empty
wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits exists and is non-empty
wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits exists and is non-empty
wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:14.676 +22:00:04.67
Second-epoch image center 10:09:05.783 +22:01:54.42
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:09:14.676 +22:00:04.67
Second-epoch image center 10:09:07.955 +22:02:00.24
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:09:05.783 +22:01:54.42
Second-epoch second image center 10:09:07.955 +22:02:00.24
Angular distance between the image centers 0.00854 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits &> /tmp/tmp.IZPZMjdL87
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits &> /tmp/tmp.8LcYj43NTF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits &> /tmp/tmp.5jkaAEyhWe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits &> /tmp/tmp.NUUF51Bhlp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
Found non-empty wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits and wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
The reference image (wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits) and catalog (wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat) found
'wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 3822 out of 30893 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.745787
a=0.000000 b=1.000000 c=22.745787
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.21
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.21
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 27 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
2.0 pix Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
2.2 pix Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
2.2 pix Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
Limiting magnitude estimates:
15.2 mag. Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
15.2 mag. Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
14.8 mag. Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
14.8 mag. Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.2 (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.IZPZMjdL87 (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-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.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-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits' -> 'wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1127, passed=30880
Got 30880 stars (including 29685 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat
util/solve_plate_with_UCAC5 got 30880 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 902 stars left (next iteration limit 992)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits -region wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-07-56_20.00sec_-15.00C_LIGHT_0255.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8LcYj43NTF (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-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.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-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits' -> 'wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1098, passed=31047
Got 31047 stars (including 29892 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat
util/solve_plate_with_UCAC5 got 31047 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 905 stars left (next iteration limit 995)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits -region wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-01-09_00-08-32_20.00sec_-15.00C_LIGHT_0256.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.5jkaAEyhWe (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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1141, passed=25355
Got 25355 stars (including 24176 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits.cat
util/solve_plate_with_UCAC5 got 25355 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 902 stars left (next iteration limit 992)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits -region wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-02-26_23-43-38_20.00sec_-14.90C_LIGHT_0089.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.NUUF51Bhlp (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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.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-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1119, passed=25434
Got 25434 stars (including 24271 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits.cat
util/solve_plate_with_UCAC5 got 25434 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 904 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: 0.35"
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 904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 903 stars left (next iteration limit 994)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-27_CI_Leo-02-Q2b1x1_044509_TTUQ2b1x1_32373_HMyckVXz/Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits -region wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090.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-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52116.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53066.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53148.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53073.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 6s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52107_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 52107_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:36:03.57 +20:14:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.400 3987341779548281728 159.01499162996 +20.23436955516 14.2084 13.6909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52108_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 52108_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:16:06.54 +24:06:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 0.729 726349475936742400 154.02724908018 +24.11010305103 14.3321 13.7823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52109_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 52109_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:39:56.26 +24:05:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.572 723348535043116032 159.98394290752 +24.09107848304 14.1549 13.2353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52111_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 52111_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 09:46:31.56 +23:42:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.637 641658016554902784 146.63221313768 +23.70414027613 13.5404 12.9544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52112_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 52112_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:24:13.78 +21:12:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 0.817 721733210727376384 156.05730465225 +21.20207618893 14.0454 13.5637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52115_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 52115_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52116_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 52116_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:25:42.18 +26:39:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 0.894 728519194631051392 156.42555313696 +26.65718593005 13.3551 12.7319 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52247_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 52247_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:23:02.84 +19:07:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 0.375 624416746518413312 155.76185311505 +19.12099140396 12.2362 11.7575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52345_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 52345_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:23:52.04 +19:34:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 0.401 624644547289308544 155.96682150483 +19.57455592321 12.8825 12.2213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52391_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 52391_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 09:42:58.04 +17:02:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 1.745 620571887499794944 145.74136033695 +17.04507553996 12.6459 12.1184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52395_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 52395_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52562_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 52562_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52568_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 52568_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52608_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 52608_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 09:59:30.80 +21:18:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 2.820 629467421899916416 149.87815754837 +21.29967854264 13.7094 13.0742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52615_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 52615_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52616_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 52616_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 09:50:55.80 +20:47:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 3.266 628064994818532608 147.73310338325 +20.78698399144 13.5849 12.9806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52639_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 52639_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52711_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 52711_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52762_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 52762_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52926_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 52926_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52930_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 52930_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53019_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 53019_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:14:42.75 +19:52:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 0.934 625332811502870656 153.67806949237 +19.87130139342 14.5357 14.0591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53066_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 53066_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:25:00.17 +20:07:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.898 624793153156688384 156.25082061033 +20.12672611530 14.7885 14.2622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53073_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 53073_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53148_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 53148_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:33:08.64 +22:34:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 2.929 721556674686893312 158.28513812535 +22.58153001264 14.8131 14.1723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.929#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53198_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 53198_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 10:12:33.15 +22:48:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 0.444 629348434126077440 153.13802495825 +22.80850139557 15.0273 14.4161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29364_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090
The candidate 29364_Leo-02-Q2b1x1_2026-02-26_23-44-24_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks