This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm
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 22.2578* 10 14 39.08 +13 16 04.6 11.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7578,11.73,0.05,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 20260222.2578 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:14:39.08 +13:16:04.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_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 22.2578* 10 03 48.36 +16 05 41.1 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7578,12.46,0.05,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 20260222.2578 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:03:48.36 +16:05:41.1 ;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-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_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 22.2578* 09 40 50.24 +18 08 29.1 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,2461093.7578,13.04,0.05,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 20260222.2578 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:40:50.24 +18:08:29.1 ;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-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_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 22.2578* 09 42 04.44 +09 43 34.2 13.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7578,13.46,0.05,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 20260222.2578 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:42:04.44 +09:43:34.2 ;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-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_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 22.2578* 09 23 33.43 +14 45 08.5 13.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7578,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2578 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:23:33.43 +14:45:08.5 ;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-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2578 2461093.7578 14.04 10:12:33.68 +09:13:25.5
230.81663 48.48694 galactic Leo Second-epoch detections are separated by 0.6" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:33.68 +09:13:25.5 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2578* 10 12 33.68 +09 13 25.5 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
target,2461093.7578,14.04,0.05,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
target 20260222.2578 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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:12:33.68 +09:13:25.5 ;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-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7578,13.87,0.05,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 20260222.2578 13.87CV 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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:18:58.75 +15:29:45.5 ;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-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2578 2461093.7578 14.06 10:14:10.13 +10:06:58.8
229.95370 49.28173 galactic Leo Second-epoch detections are separated by 2.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:14:10.13 +10:06:58.8 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2578* 10 14 10.13 +10 06 58.8 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7578,14.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2578 14.06CV 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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:14:10.13 +10:06:58.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_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 22.2578* 10 06 04.95 +15 21 33.7 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7578,14.05,0.05,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 20260222.2578 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:06:04.95 +15:21:33.7 ;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-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2578 2461093.7578 14.10 10:12:40.82 +10:07:24.7
229.66341 48.96841 galactic Leo Second-epoch detections are separated by 2.0" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:12:40.82 +10:07:24.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2578* 10 12 40.82 +10 07 24.7 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7578,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2578 14.10CV 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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:12:40.82 +10:07:24.7 ;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-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2578 2461093.7578 14.37 10:14:56.86 +10:05:58.1
230.12424 49.43886 galactic Leo Second-epoch detections are separated by 3.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:14:56.86 +10:05:58.1 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2578* 10 14 56.86 +10 05 58.1 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
target,2461093.7578,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2578 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:14:56.86 +10:05:58.1 ;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-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_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 22.2578* 10 15 18.02 +10 02 28.7 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
Gaia DR3 3876751834874176128,2461093.7578,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3876751834874176128 20260222.2578 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:15:18.02 +10:02:28.7 ;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-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_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 22.2578* 10 00 16.15 +17 50 13.6 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,2461093.7578,14.39,0.05,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 20260222.2578 14.39CV 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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:00:16.15 +17:50:13.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_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 22.2578* 09 34 58.68 +14 46 52.3 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,2461093.7578,14.40,0.05,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 20260222.2578 14.40CV 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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:34:58.68 +14:46:52.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20_00sec_-14_90C_LIGHT_0207_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: 2461049.73802228 09.01.2026 05:42:35.125 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
First image: 2461049.73802228 09.01.2026 05:42:35.125 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Last image: 2461093.75809155 22.02.2026 06:11:29.110 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 60
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.75
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: 5 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): 8250
Objects passed selection criteria: 8243
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 7311.5
Average stars matched: 6686 (91.445 %)
Memory usage VmPeak: 113636 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 Sun Feb 22 06:24:56 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: 2461049.73802228 09.01.2026 05:42:35.125 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
First image: 2461049.73802228 09.01.2026 05:42:35.125 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Last image: 2461093.75809155 22.02.2026 06:11:29.110 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 149
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
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: 19 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): 42786
Objects passed selection criteria: 42696
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: 40368.8
Average stars matched: 36961.2 (91.5591 %)
Memory usage VmPeak: 142272 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 Sun Feb 22 06:26:08 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-04-Q2b1x1
#######################################
########### Starting Leo-04-Q2b1x1 ###########
Processing Leo-04-Q2b1x1
server tau has sufficient free disk space available: 984101 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 984101 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.png' -> 'transient_report/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits_preview.png'
Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
renamed 'Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.png' -> 'transient_report/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits_preview.png'
Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.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= 799.0258
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 530.4221
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1018.7968
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 565.8808
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1018.4582
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 565.3987
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 1.27505
INFO: SECOND_EPOCH__SD_ratio= 0.001
----------------------------------------------
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_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
No bad regions file found ../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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
SExtractor catalog cache: saved Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.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: 2461093.75756362
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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits exists and is non-empty
Saving wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits to local_wcs_cache/
'wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits' -> 'local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits'
wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits exists and is non-empty
Saving wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits to local_wcs_cache/
'wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits' -> 'local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits'
wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits exists and is non-empty
Saving wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits to local_wcs_cache/
'wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits' -> 'local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits'
wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits exists and is non-empty
Saving wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits to local_wcs_cache/
'wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits' -> 'local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.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 09:46:15.747 +13:59:46.03
Second-epoch image center 09:46:34.263 +14:02:41.10
Angular distance between the image centers 0.09 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 09:46:15.747 +13:59:46.03
Second-epoch image center 09:46:34.374 +14:02:15.67
Angular distance between the image centers 0.09 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 09:46:34.263 +14:02:41.10
Second-epoch second image center 09:46:34.374 +14:02:15.67
Angular distance between the image centers 0.00708 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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits &> /tmp/tmp.VTzsT5THO3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits &> /tmp/tmp.4W9UKPTk31
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits &> /tmp/tmp.6u3HibbLkB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits &> /tmp/tmp.pC9vbB6Uuu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits and wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits and wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
Found non-empty wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits and wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
The reference image (wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits) and catalog (wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat) found
'wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.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 4091 out of 6614 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.851468
a=0.000000 b=1.000000 c=22.851468
From vast_summary.log: estimated ref. image limiting mag.: -7.75
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.10
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.10
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 59 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
2.0 pix Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
2.4 pix Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
2.4 pix Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
Limiting magnitude estimates:
15.1 mag. Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
15.1 mag. Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
15.2 mag. Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
15.3 mag. Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.VTzsT5THO3 (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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.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_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits' -> 'wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=440, passed=6614
Got 6614 stars (including 6163 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
util/solve_plate_with_UCAC5 got 6614 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.26"
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 911 stars left (next iteration limit 1002)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits -region wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.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.4W9UKPTk31 (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-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.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_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.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-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.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-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits' -> 'wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=457, passed=6505
Got 6505 stars (including 6040 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat
util/solve_plate_with_UCAC5 got 6505 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 914 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits -region wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.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.6u3HibbLkB (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_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.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_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=648, passed=8145
Got 8145 stars (including 7490 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits.cat
util/solve_plate_with_UCAC5 got 8145 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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: 0.35"
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 913 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: 0.37"
Excluding outliers - 913 stars left (next iteration limit 1004)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits -region wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.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.pC9vbB6Uuu (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_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.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_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=629, passed=8144
Got 8144 stars (including 7510 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 8144 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 913 stars left (next iteration limit 1004)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits -region wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.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-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20446.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20498.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out20480.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out20401.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 20274_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20274_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:14:57.62 +09:12:38.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20401_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
Preparing report for the candidate 20401_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
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Considering the candidate 20410_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20410_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:40:58.96 +09:52:39.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 20411_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20411_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:42:27.62 +13:47:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 0.524 614599202898529408 145.61522039345 +13.78842011641 12.1072 11.6743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20418_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20418_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:40:52.29 +14:14:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.350 617768029769833728 145.21783901811 +14.23435360583 12.0399 11.5401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20427_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20427_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:36:21.46 +13:37:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 0.872 617267034719616768 144.08918255539 +13.62275017881 11.9521 11.3367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20431_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20431_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:47:19.89 +12:53:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 0.454 614339207053944576 146.83284461324 +12.89403922255 12.0746 11.4125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20440_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20440_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:45:28.13 +15:40:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 1.285 619478221322493952 146.36756453388 +15.68151542671 12.1154 11.3146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20442_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20442_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:43:45.94 +12:46:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.647 614278562115535744 145.94126388754 +12.77348950344 12.2217 11.7817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20443_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20443_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:00:29.83 +15:50:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.728 616634605080128128 150.12419399523 +15.84648747856 12.2516 11.5510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20445_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20445_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:48:36.26 +13:48:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.756 615957000975263488 147.15088355406 +13.81522545216 12.2595 11.8339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20446_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20446_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:45:17.89 +12:40:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.302 614237532292399104 146.32456446376 +12.67369701834 12.2157 11.7505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20449_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20449_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:47:43.99 +14:45:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.168 616262901430224384 146.93331119769 +14.76276301603 12.2820 11.7885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20450_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20450_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:44:38.57 +11:41:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.650 613037518429884288 146.16065329550 +11.69781109808 12.1316 11.5058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.650#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20452_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20452_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:36:59.70 +13:21:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.333 617241776016698240 144.24865746802 +13.35742377583 12.1979 11.7889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20453_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20453_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:50:22.35 +13:04:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.622 613611875816449792 147.59306351829 +13.07935651362 12.2265 11.7241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20454_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20454_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:45:21.68 +14:51:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.598 619260307566733952 146.34023477215 +14.85641377115 12.2301 11.8045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20455_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20455_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:42:44.59 +11:45:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.787 613770446009341184 145.68565025812 +11.75061364390 12.1844 11.7101 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#
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Considering the candidate 20456_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20456_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:38:31.37 +13:15:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.288 617183020863980288 144.63079045295 +13.25363400559 12.1481 11.6117 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#
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Considering the candidate 20457_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20457_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:15:14.10 +09:06:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 1.730 3876526022673706880 153.80835595847 +09.10844863272 11.3455 11.0286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20458_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20458_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:44:28.94 +11:48:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.507 613042500591945856 146.12052194543 +11.81534957647 12.2938 11.7281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20459_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20459_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:38:37.74 +12:01:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.327 613946024272411776 144.65717366343 +12.02991295011 12.1031 11.4459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20460_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20460_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:48:53.57 +13:35:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.554 614437441545857664 147.22308953529 +13.58471268030 12.3343 11.9126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20462_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20462_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:39:55.10 +14:30:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.674 617790260520553856 144.97974943962 +14.50398753633 12.2458 11.7914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20463_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20463_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:42:51.84 +14:39:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.528 617811254320303360 145.71608500066 +14.65523243494 12.2676 11.7770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20465_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20465_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:43:16.89 +11:20:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.822 612990170710421632 145.82021843400 +11.34014131780 12.0823 11.3714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20466_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20466_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:43:42.09 +11:50:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 1.068 613793260875616000 145.92510479503 +11.84424554648 12.1998 11.6379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20468_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20468_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:38:39.42 +12:27:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.459 614063912534411136 144.66420568489 +12.45220338797 12.1482 11.5162 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20469_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20469_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:47:02.83 +14:51:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.465 616279707637729152 146.76183927835 +14.85528745967 12.2487 11.6258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20470_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20470_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:49:38.03 +13:21:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.602 614383118799547136 147.40830349574 +13.36310040118 12.3345 11.8889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20472_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20472_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:46:04.50 +11:45:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.347 613030165446238336 146.51865888317 +11.75525845349 12.2897 11.8413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20473_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20473_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:42:58.00 +15:20:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.545 619536147546331776 145.74176075054 +15.33767667965 12.2239 11.6766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20474_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20474_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:35:53.53 +15:22:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.150 618842183910404352 143.97301034073 +15.36897310916 12.1762 11.7023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20475_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20475_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:44:17.52 +12:45:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.812 614266222673934208 146.07298463770 +12.75350288397 12.2660 11.6623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20476_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20476_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:46:38.55 +14:04:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.067 614666410547216896 146.66063132645 +14.06723255377 12.4020 11.9676 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20477_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20477_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:36:28.38 +12:38:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.655 617040123007669248 144.11825230590 +12.64387623672 12.1875 11.6231 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#
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Considering the candidate 20479_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20479_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:48:09.20 +11:14:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.180 612764908265670016 147.03828305728 +11.24424132536 12.2515 11.7808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20480_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20480_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:40:22.59 +14:57:32.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)
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Considering the candidate 20481_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20481_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:51:23.95 +13:39:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.816 615884433207851008 147.84961267231 +13.66258995032 12.5272 12.0339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20482_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20482_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:52:20.02 +10:48:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.609 3879654442492651008 148.08331657397 +10.80074886164 12.1941 11.6633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20485_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20485_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:42:25.21 +11:46:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.060 613771412377298176 145.60504724497 +11.76903989875 12.2253 11.6126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20486_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20486_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:45:32.50 +16:23:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.450 619727737447257472 146.38538659722 +16.39631596372 12.2357 11.7121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20487_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20487_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:53:36.59 +13:05:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.416 615052923243773696 148.40252564701 +13.09984502936 12.2902 11.8274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20488_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20488_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:49:41.94 +13:38:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.197 615893023142412160 147.42470055568 +13.64852943727 12.3862 11.9684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20489_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20489_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:54:08.93 +12:38:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 0.612 614835907137012608 148.53725052419 +12.64235925386 12.2210 11.6032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20490_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20490_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:46:05.43 +12:40:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.426 614235234485482112 146.52264503717 +12.66878327997 12.3253 11.7813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20491_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20491_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:41:45.16 +12:01:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 0.556 613838791824197376 145.43819186555 +12.02270792648 12.2410 11.5376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20492_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20492_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:46:19.03 +12:17:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.354 613439252490879616 146.57919489254 +12.28497148301 12.2666 11.4958 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20494_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20494_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:51:20.00 +13:52:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.482 615926661326237696 147.83320240275 +13.88054250030 12.3866 11.9324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20495_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20495_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:36:40.28 +14:43:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.112 617950754858243456 144.16781566996 +14.72619624750 12.2811 11.8658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20497_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20497_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:44:05.77 +11:31:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.983 612999138602132096 146.02388830514 +11.51820006285 12.2910 11.8119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20498_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20498_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:45:06.85 +15:47:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.703 619668088941457024 146.27835063189 +15.79953774551 12.2802 11.7042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20499_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20499_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:48:53.55 +15:26:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.867 619398536793960960 147.22310950811 +15.44387925714 12.3510 11.8907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20500_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20500_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:40:21.29 +13:15:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.064 614551378437643392 145.08870313828 +13.26337827794 12.2234 11.5068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20501_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20501_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:51:10.91 +15:06:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 1.006 616347632545341312 147.79558499082 +15.11541808732 12.2859 11.6678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.006#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20503_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20503_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:36:47.99 +13:48:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.659 617648732758429952 144.19991751530 +13.81545660874 12.2876 11.7533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20504_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20504_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:43:03.87 +11:46:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.426 613772232715735552 145.76607919914 +11.77983170240 12.3726 11.9198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20505_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20505_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:49:18.28 +15:12:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.223 616388005238255872 147.32620973517 +15.20124050032 12.2598 11.6040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20506_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 20506_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:38:26.83 +11:54:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.296 613936128667767040 144.61172694812 +11.91235781097 12.2767 11.8098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Leo-04-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 ####
10:14:39.08 +13:16:04.6
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
SExtractor catalog cache: saved Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Creating symlink local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
Creating symlink local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
Creating symlink local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits exists and is non-empty
wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits exists and is non-empty
wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits exists and is non-empty
wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.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 09:46:15.747 +13:59:46.03
Second-epoch image center 09:46:34.263 +14:02:41.10
Angular distance between the image centers 0.09 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 09:46:15.747 +13:59:46.03
Second-epoch image center 09:46:34.374 +14:02:15.67
Angular distance between the image centers 0.09 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 09:46:34.263 +14:02:41.10
Second-epoch second image center 09:46:34.374 +14:02:15.67
Angular distance between the image centers 0.00708 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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits &> /tmp/tmp.91yKfPekp2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits &> /tmp/tmp.NjY6x2BO1o
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits &> /tmp/tmp.kxRko6UiKq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits &> /tmp/tmp.MKItXw5uYU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits and wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits and wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
Found non-empty wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits and wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
The reference image (wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits) and catalog (wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat) found
'wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.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 4172 out of 37606 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.734542
a=0.000000 b=1.000000 c=22.734542
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.24
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.24
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 63 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
1.9 pix Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
2.3 pix Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
2.3 pix Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
Limiting magnitude estimates:
15.2 mag. Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
15.3 mag. Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
15.5 mag. Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
15.5 mag. Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.91yKfPekp2 (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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.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_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits' -> 'wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1467, passed=37598
Got 37598 stars (including 36067 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
util/solve_plate_with_UCAC5 got 37598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 909 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: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 909 stars left (next iteration limit 999)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits -region wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.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.NjY6x2BO1o (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-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.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_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.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-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.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-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits' -> 'wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1514, passed=38235
Got 38235 stars (including 36667 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat
util/solve_plate_with_UCAC5 got 38235 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 909 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: 0.28"
Excluding outliers - 909 stars left (next iteration limit 999)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits -region wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.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.kxRko6UiKq (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_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.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_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=2390, passed=43424
Got 43424 stars (including 40984 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits.cat
util/solve_plate_with_UCAC5 got 43424 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 912 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 912 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: 0.36"
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-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits -region wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-02-22_00-10-43_20.00sec_-14.90C_LIGHT_0207.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.MKItXw5uYU (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_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.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_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=2379, passed=43365
Got 43365 stars (including 40938 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 43365 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
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-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Leo-04-Q2b1x1_001219_TTUQ2b1x1_23112_gmta1evm/Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits -region wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208.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-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53031.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54179.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54606.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 23s
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: 8s
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Considering the candidate 53011_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53011_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:17:38.67 +16:27:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.925 631691081088475648 139.41167756935 +16.45448718935 13.7514 13.2423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53019_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53019_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:50:43.51 +10:30:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.207 3879267616262463872 147.68106493550 +10.51236155092 14.2841 13.7584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53023_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53023_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:59:43.87 +18:19:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 0.308 626202422121192704 149.93285685315 +18.32688532111 14.3470 13.7017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53024_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53024_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:11:18.15 +09:51:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.759 3876871711706095360 152.82611762688 +09.85402789823 13.2628 12.7529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53025_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53025_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:43:17.54 +17:01:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 0.991 620574606214378112 145.82287278281 +17.03046560404 14.2626 13.8164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.991#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53028_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53028_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:16:42.57 +17:26:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.850 632083812897779072 139.17686719783 +17.43438401818 13.1595 12.7070 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53031_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53031_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:51:07.09 +16:14:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 0.223 619861847801432064 147.77960474644 +16.24042934627 13.3208 12.6788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53034_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53034_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:58:14.72 +14:48:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 0.319 615714313847462528 149.56127529703 +14.80295759442 12.7445 12.3448 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53038_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53038_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:13:30.41 +09:11:09.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53041_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53041_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:14:57.63 +09:12:38.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53194_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53194_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:14:39.09 +13:16:04.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53252_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53252_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:15:11.71 +09:08:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.494 3876537872488073216 153.79917235764 +09.13546304230 11.1505 10.5760 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53258_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53258_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:15:14.09 +09:06:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 1.612 3876526022673706880 153.80835595847 +09.10844863272 11.3455 11.0286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53323_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
Preparing report for the candidate 53323_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
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Considering the candidate 53340_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53340_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:15:24.37 +09:27:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 0.395 3876646419196889344 153.85160057047 +09.45420424262 11.5973 11.0655 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53373_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53373_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:39:00.87 +14:25:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.060 617883860743199360 144.75343225598 +14.43244987355 12.9679 12.4398 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53382_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53382_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:13:26.56 +09:25:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.993 3876608000714651008 153.35982992408 +09.42568232586 11.5170 10.9251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53467_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53467_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:15:30.99 +09:28:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.536 3876646861578183168 153.87899948137 +09.47894405344 12.0495 11.5581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53499_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53499_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:13:37.54 +08:58:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.493 3876531172339395968 153.40607745206 +08.96882774984 11.9969 11.4115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53538_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
Preparing report for the candidate 53538_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
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Considering the candidate 53619_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53619_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:15:55.90 +09:43:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.229 3876721735743383680 153.98261597054 +09.71841957637 12.4337 12.0143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53642_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53642_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:13:44.27 +09:25:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.404 3876608211167823488 153.43360979605 +09.42635621290 12.2129 11.7371 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53649_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
Preparing report for the candidate 53649_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
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Considering the candidate 53652_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53652_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:13:11.01 +08:53:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 4.952 3876506815579983488 153.29453700035 +08.89018547354 12.0226 11.3540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.952#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53674_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53674_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:16:16.34 +10:17:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 3.906 3877320076227325952 154.06704429593 +10.29755760365 12.6428 12.2575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53786_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53786_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:15:36.38 +09:01:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.332 3876521414173698816 153.90126896485 +09.02542333701 12.4063 11.9150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53847_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
Preparing report for the candidate 53847_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
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Considering the candidate 53856_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53856_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:14:44.89 +09:49:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 3.374 3876718226755348224 153.68630059008 +09.82686546030 12.6447 12.1599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53864_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53864_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:15:55.16 +09:07:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 0.571 3876616285706374912 153.97988824130 +09.12706581347 12.7629 12.2649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53876_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53876_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:15:38.32 +09:44:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 3.936 3876724965558791936 153.90857967371 +09.73732866830 12.7025 12.2554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.936#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53912_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53912_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:15:40.79 +09:28:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 0.461 3876646694074793856 153.91982970351 +09.47512060513 12.9414 12.5305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53918_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 53918_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:30:14.24 +12:51:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.655 617292735804075520 142.55937206326 +12.85473364937 14.0324 13.6238 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#
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Considering the candidate 53979_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
Preparing report for the candidate 53979_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
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Considering the candidate 53993_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
Preparing report for the candidate 53993_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
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Considering the candidate 54010_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
Preparing report for the candidate 54010_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
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Considering the candidate 54033_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54033_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:14:14.99 +09:12:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.323 3876542996384466432 153.56212092364 +09.21484999991 12.9144 12.4182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54040_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54040_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:15:44.48 +10:45:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 3.937 3877352404446090752 153.93423492017 +10.75584330142 13.0593 12.5258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54085_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54085_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:15:05.38 +09:06:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.771 3876525953954231168 153.77192610909 +09.10613702166 12.8530 12.3258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54087_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
Preparing report for the candidate 54087_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
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Considering the candidate 54101_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54101_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:12:42.74 +09:28:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 3.934 3876611647141656704 153.17709375200 +09.47174121995 12.9938 12.4633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54113_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54113_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:11:21.66 +09:24:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 4.140 3876794539733731584 152.83909857617 +09.40037290776 13.1732 12.5538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54135_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
Preparing report for the candidate 54135_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
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Considering the candidate 54179_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54179_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:11:51.50 +09:16:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 3.911 3876602095134419584 152.96351552074 +09.27940239037 13.3657 12.8445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54252_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54252_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:05:21.51 +15:35:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 1.715 621831107486841984 151.33935242697 +15.58686970845 14.3695 13.7900 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54258_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54258_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:14:03.24 +09:17:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.081 3876591237457069952 153.51320776349 +09.28683388371 13.4152 12.9036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54266_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54266_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:14:04.96 +09:18:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 2.826 3876591271816807552 153.51989279269 +09.30576529356 13.2895 12.7546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54298_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
Preparing report for the candidate 54298_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
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Considering the candidate 54331_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
Preparing report for the candidate 54331_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54337_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54337_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:15:23.95 +09:15:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.049 3876635007468451072 153.84956658770 +09.26318853294 13.4028 12.9683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54339_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54339_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:58:09.41 +13:26:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 0.311 615006335733637376 149.53918919647 +13.45002873613 14.8138 14.2638 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54389_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
Preparing report for the candidate 54389_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
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Considering the candidate 54393_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54393_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:51:52.94 +12:57:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 3.331 613592222046106368 147.97033409654 +12.95192065467 15.0933 14.4755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54396_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54396_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:38:04.44 +13:50:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.222 617640834313399552 144.51846968956 +13.84211595489 14.5637 13.8922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54454_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54454_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 09:32:00.01 +09:40:56.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54488_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54488_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:12:44.23 +09:03:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 2.781 3876556877718721280 153.18350952916 +09.05226909591 13.2560 12.7813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54489_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 54489_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
**** FOUND 10:13:33.00 +08:52:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 1.908 3876503757563265792 153.38702580528 +08.86827570175 13.3812 12.9886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54606_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
Preparing report for the candidate 54606_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
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Considering the candidate 37099_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 37099_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 28599_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 28599_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 15445_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 15445_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
Rejecting candidate due to large distance (25.3") between the two second-epoch detections
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Considering the candidate 29128_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 29128_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 22974_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 22974_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
Rejecting candidate due to large distance (24.9") between the two second-epoch detections
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Considering the candidate 09495_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208
The candidate 09495_Leo-04-Q2b1x1_2026-02-22_00-11-29_20.00sec_-15.00C_LIGHT_0208 did not pass the final checks
