This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP
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 03 19.3533* 11 22 42.75 +02 22 15.3 10.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8533,10.79,0.05,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 20260319.3533 10.79CV 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:22:42.75 +02:22:15.3 ;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-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_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 03 19.3533* 10 47 09.08 +00 04 25.2 11.5 U Sex 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,2461118.8533,11.50,0.05,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 20260319.3533 11.50CV 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:47:09.08 -00:04:25.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_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 03 19.3533* 11 30 34.97 +00 22 55.5 11.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8533,11.87,0.05,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 20260319.3533 11.87CV 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:30:34.97 +00:22:55.5 ;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-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_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 03 19.3533* 11 10 22.19 +01 07 51.8 12.1 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,2461118.8533,12.05,0.05,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 20260319.3533 12.05CV 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:10:22.19 +01:07:51.8 ;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-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_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 03 19.3533* 10 49 15.18 +02 22 06.8 12.9 U Sex 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,2461118.8533,12.87,0.05,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 20260319.3533 12.87CV 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:49:15.18 +02:22:06.8 ;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-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_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 03 19.3533* 10 52 20.58 -02 34 14.2 13.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8533,13.18,0.05,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 20260319.3533 13.18CV 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:52:20.58 -02:34:14.2 ;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-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_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 03 19.3533* 11 01 32.85 -05 43 07.6 13.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8533,13.89,0.05,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 20260319.3533 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:01:32.85 -05:43:07.6 ;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-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3533 2461118.8533 14.14 11:31:32.06 -02:18:32.7
266.59493 54.82460 galactic Leo Second-epoch detections are separated by 4.3" and 2.4 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 | ATO J172.8835-02.3093 | 11:31:32.06 -02:18:32.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.054+/-0.158 (M)
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 03 19.3533* 11 31 32.06 -02 18 32.7 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
ATO J172.8835-02.3093,2461118.8533,14.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J172.8835-02.3093 20260319.3533 14.14CV 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:31:32.06 -02:18:32.7 ;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-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20_00sec_-15_00C_LIGHT_0087_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20_00sec_-14_90C_LIGHT_0455_fits__*pix.png resample_wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20_00sec_-14_90C_LIGHT_0086_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
First image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Last image: 2461118.85354072 19.03.2026 08:28:55.918 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6634
Objects passed selection criteria: 6632
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 6322.25
Average stars matched: 6128.75 (96.9394 %)
Memory usage VmPeak: 112568 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 03:37:57 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
First image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Last image: 2461118.85354072 19.03.2026 08:28:55.918 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 296
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 10 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 34437
Objects passed selection criteria: 34361
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 32757.5
Average stars matched: 31709.8 (96.8015 %)
Memory usage VmPeak: 135564 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 03:38:43 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
SExtractor catalog cache: saved Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat to cache
SExtractor catalog cache: saved Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.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: 2461118.85301076
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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits exists and is non-empty
Saving wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits to local_wcs_cache/
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits exists and is non-empty
Saving wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits to local_wcs_cache/
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits exists and is non-empty
Saving wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits to local_wcs_cache/
'wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits' -> 'local_wcs_cache/wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits'
wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits exists and is non-empty
Saving wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits to local_wcs_cache/
'wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits' -> 'local_wcs_cache/wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:45.891 -01:55:56.79
Angular distance between the image centers 0.08 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:45.420 -01:55:50.57
Angular distance between the image centers 0.08 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:45.891 -01:55:56.79
Second-epoch second image center 11:08:45.420 -01:55:50.57
Angular distance between the image centers 0.00261 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits &> /tmp/tmp.63jyWEvZiu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits &> /tmp/tmp.tIDYsrCaX2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits &> /tmp/tmp.07H8ExAlkT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits &> /tmp/tmp.CkngdU7Sor
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Found non-empty wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
The reference image (wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits) and catalog (wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat) found
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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 3372 out of 6399 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.879752
a=0.000000 b=1.000000 c=22.879752
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
2.2 pix Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
2.4 pix fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
2.3 pix fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
Limiting magnitude estimates:
15.2 mag. Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
15.2 mag. Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
15.1 mag. fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
15.1 mag. fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.63jyWEvZiu (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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=432, passed=6399
Got 6399 stars (including 5960 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
util/solve_plate_with_UCAC5 got 6399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 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 - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits -region wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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.tIDYsrCaX2 (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-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=407, passed=6519
Got 6519 stars (including 6107 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
util/solve_plate_with_UCAC5 got 6519 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 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: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits -region wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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.07H8ExAlkT (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_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.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_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
Checking if the catalog wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
WCS catalog name: wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=376, passed=6321
Got 6321 stars (including 5942 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits.cat
util/solve_plate_with_UCAC5 got 6321 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits -region wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.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.CkngdU7Sor (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_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.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_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
Checking if the catalog wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
WCS catalog name: wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=391, passed=6222
Got 6222 stars (including 5827 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat
util/solve_plate_with_UCAC5 got 6222 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits -region wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
Saving fully-calibrated image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
Saving fully-calibrated image wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits'
Saving fully-calibrated image wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits'
Preparing the HTML report for the field Leo-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20425.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20396_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 20396_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20406_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 20406_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20420_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 20420_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20425_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 20425_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20427_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 20427_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:00:24.17 -02:42:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.697 3801762663667379968 165.10089962507 -02.70733738931 12.1730 11.8880 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.697#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-08-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 ####
11:22:42.75 +02:22:15.3
10:47:09.08 -00:04:25.2
11:30:34.97 +00:22:55.5
11:10:22.19 +01:07:51.8
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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
SExtractor catalog cache: saved Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat to cache
SExtractor catalog cache: saved Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Creating symlink local_wcs_cache/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits exists and is non-empty
wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits exists and is non-empty
wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits exists and is non-empty
wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:45.891 -01:55:56.79
Angular distance between the image centers 0.08 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:45.420 -01:55:50.57
Angular distance between the image centers 0.08 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:45.891 -01:55:56.79
Second-epoch second image center 11:08:45.420 -01:55:50.57
Angular distance between the image centers 0.00261 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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits &> /tmp/tmp.cLIU9rEUV0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits &> /tmp/tmp.PjaEiM25l7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits &> /tmp/tmp.i1kgbZUdnO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits &> /tmp/tmp.gv2leeu8n4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Found non-empty wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
The reference image (wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits) and catalog (wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat) found
'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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 3398 out of 34371 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.774901
a=0.000000 b=1.000000 c=22.774901
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 176 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
2.2 pix Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
2.4 pix fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
2.2 pix fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
Limiting magnitude estimates:
15.3 mag. Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
15.3 mag. Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
15.2 mag. fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
15.3 mag. fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.5 (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.cLIU9rEUV0 (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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1404, passed=34365
Got 34365 stars (including 32904 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
util/solve_plate_with_UCAC5 got 34365 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits -region wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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.PjaEiM25l7 (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-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Checking if the catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS catalog name: wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1420, passed=33111
Got 33111 stars (including 31640 good ones) from the SExtractor catalog wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
util/solve_plate_with_UCAC5 got 33111 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits -region wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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.i1kgbZUdnO (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_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.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_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
Checking if the catalog wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
WCS catalog name: wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=1281, passed=31779
Got 31779 stars (including 30461 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits.cat
util/solve_plate_with_UCAC5 got 31779 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits -region wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.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.gv2leeu8n4 (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_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.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_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
Checking if the catalog wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
WCS catalog name: wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1371, passed=32794
Got 32794 stars (including 31395 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat
util/solve_plate_with_UCAC5 got 32794 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits -region wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Saving fully-calibrated image wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/wcs_Leo-08-Q2b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Saving fully-calibrated image wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-10_20.00sec_-14.90C_LIGHT_0086.fits
Saving fully-calibrated image wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-08-Q2b1x1_033548_TTUQ2b1x1_12734_1cKZW5KP/wcs_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087.fits
Preparing the HTML report for the field Leo-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out51842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52170.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 51719_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51719_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:32:20.23 -01:34:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 4.849 3793694760872123776 173.08391890186 -01.57051652448 14.5655 14.0562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.849#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51725_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51725_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 10:55:15.19 -00:48:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 1.438 3803000889850806016 163.81368755172 -00.81638701142 14.1230 13.6785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51726_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51726_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 10:39:10.59 +02:05:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 2.705 3855797410991828480 159.79460778938 +02.08367395306 13.5271 12.9306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51729_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51729_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:32:30.19 +00:00:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51730_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51730_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:25:45.76 +01:30:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.286 3798666889892019072 171.44092006622 +01.51519270313 13.5158 12.8799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51731_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51731_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:38:08.68 -03:30:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 0.799 3792267422980803456 174.53631758723 -03.51666283326 13.5121 12.8831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51733_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51733_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:38:24.89 +02:04:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.511 3799326253271455232 174.60368193568 +02.08152719552 13.5896 13.0593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51734_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51734_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:21:44.37 -05:56:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.204 3785648981456834304 170.43492606668 -05.94433597436 13.2293 12.6797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51737_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51737_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:34:19.10 -03:15:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51761_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51761_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:22:42.75 +02:22:15.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 51775_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51775_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 10:47:09.08 -00:04:25.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 51791_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51791_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:30:34.98 +00:22:55.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 51792_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51792_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:06:45.00 +01:57:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.477 3811456477865625216 166.68762346724 +01.96214621979 11.8047 11.2892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51796_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51796_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:10:22.19 +01:07:51.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 51797_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51797_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 51799_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51799_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51808_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51808_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 51814_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51814_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 51827_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51827_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 51830_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51830_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 51842_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 51842_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 51845_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51845_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 51848_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51848_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 51854_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51854_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 51855_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51855_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 51858_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51858_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 51859_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51859_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 51860_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51860_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51861_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51861_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 51862_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51862_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 51868_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51868_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 51871_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51871_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 51873_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51873_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51874_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51874_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 51879_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 51879_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 51882_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51882_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 51883_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51883_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51889_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51889_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 51891_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51891_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51892_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51892_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 51893_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51893_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51901_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51901_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 51903_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51903_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 51914_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51914_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 51919_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51919_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 51920_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51920_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 51921_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51921_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 51922_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51922_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 51926_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51926_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 51927_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51927_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 51928_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51928_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 51929_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51929_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 51930_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51930_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 51933_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51933_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 51938_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51938_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 51943_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51943_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 51944_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51944_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 51945_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51945_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51946_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51946_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 51949_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51949_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 51951_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51951_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 51952_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51952_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51956_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51956_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 51957_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51957_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51959_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51959_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 51960_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51960_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 51966_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51966_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51967_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51967_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51968_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51968_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51973_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51973_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 51974_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51974_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 51976_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51976_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51980_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51980_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 51981_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51981_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 51982_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51982_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 51988_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51988_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51991_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51991_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 51992_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51992_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 51997_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51997_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 51998_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51998_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 51999_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 51999_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52000_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52000_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52001_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52001_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52002_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52002_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52010_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52010_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52012_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52012_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52013_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52013_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 52015_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52015_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 52017_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52017_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 52021_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52021_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 52022_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52022_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52026_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52026_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52028_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52028_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52029_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52029_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52030_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52030_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 52037_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52037_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52041_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52041_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52042_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52042_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52046_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52046_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52047_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52047_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 52048_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52048_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 52051_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52051_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52052_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 52052_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 52054_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52054_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52057_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52057_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 52060_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52060_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 52062_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52062_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 52066_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52066_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52067_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52067_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 52072_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52072_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 52074_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52074_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 52075_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52075_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52076_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52076_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52077_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52077_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 52079_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52079_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 52081_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52081_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52084_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52084_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52089_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52089_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52090_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52090_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52096_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52096_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 10:51:36.71 -02:35:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 0.528 3801591552166674944 162.90308416205 -02.59796471367 13.9426 13.4703 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 52098_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52098_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52100_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52100_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:37:10.29 -00:48:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.334 3794172739192770304 174.29346247727 -00.80963539223 14.0524 13.4427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.334#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52107_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52107_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 52109_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52109_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52110_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52110_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52114_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52114_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52116_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52116_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52119_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52119_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52120_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52120_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52121_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52121_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 52122_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52122_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52124_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52124_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 52125_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52125_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52126_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52126_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 52128_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52128_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 52132_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52132_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52133_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52133_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52137_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52137_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52145_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52145_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52152_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52152_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52153_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52153_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:26:50.74 +01:39:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.791 3798675136229258368 171.71144753215 +01.66367023460 14.1818 13.6700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52154_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52154_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52157_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52157_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52159_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52159_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52164_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52164_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52165_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52165_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 52166_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52166_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52170_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 52170_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 52173_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52173_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52175_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52175_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52182_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52182_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52184_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52184_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52186_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52186_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52189_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52189_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 52202_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52202_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52203_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52203_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52207_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52207_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52213_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52213_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52218_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52218_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52221_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52221_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52223_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52223_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52236_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52236_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52237_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52237_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52238_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52238_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:39:49.05 +02:21:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.072 3799712422370764544 174.95464411664 +02.35128845108 14.2868 13.8886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52244_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52244_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52246_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52246_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52251_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52251_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52258_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52258_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52262_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52262_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 52267_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52267_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 11:31:18.88 -06:36:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.707 3593251351587336320 172.82907960966 -06.60090424233 14.4193 13.9483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52269_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52269_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 52296_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52296_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 52297_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52297_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52320_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52320_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52345_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 52345_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 33854_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087
The candidate 33854_fd_Leo-08-Q2b1x1_2026-03-19_03-28-55_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks