This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN
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 22.3129* 11 18 04.50 +09 06 15.5 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.8129,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3129 12.79CV 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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:18:04.50 +09:06:15.5 ;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-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20_00sec_-15_00C_LIGHT_0174_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20_00sec_-14_90C_LIGHT_0173_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20_00sec_-15_00C_LIGHT_0174_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20_00sec_-14_90C_LIGHT_0173_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 22.3129* 11 58 08.61 +13 09 36.5 12.9 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,2461121.8129,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3129 12.91CV 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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:58:08.61 +13:09:36.5 ;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-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20_00sec_-15_00C_LIGHT_0174_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20_00sec_-14_90C_LIGHT_0173_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20_00sec_-15_00C_LIGHT_0174_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20_00sec_-14_90C_LIGHT_0173_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 22.3129* 11 19 30.76 +09 35 26.4 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.8129,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3129 14.07CV 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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:19:30.76 +09:35:26.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20_00sec_-15_00C_LIGHT_0174_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20_00sec_-14_90C_LIGHT_0173_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20_00sec_-15_00C_LIGHT_0174_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20_00sec_-14_90C_LIGHT_0173_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 22.3129* 12 03 42.40 +09 34 16.2 14.6 U Vir 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,2461121.8129,14.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3129 14.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:03:42.40 +09:34:16.2 ;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-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20_00sec_-15_00C_LIGHT_0174_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20_00sec_-14_90C_LIGHT_0173_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20_00sec_-15_00C_LIGHT_0174_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20_00sec_-14_90C_LIGHT_0173_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 22.3129* 11 43 54.30 +17 32 28.8 14.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.8129,14.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3129 14.72CV 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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:43:54.30 +17:32:28.8 ;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-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20_00sec_-15_00C_LIGHT_0174_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20_00sec_-14_90C_LIGHT_0173_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20_00sec_-15_00C_LIGHT_0174_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20_00sec_-14_90C_LIGHT_0173_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 22.3129* 11 52 00.00 +18 57 24.3 14.8 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,2461121.8129,14.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3129 14.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:52:00.00 +18:57:24.3 ;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-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20_00sec_-15_00C_LIGHT_0174_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20_00sec_-14_90C_LIGHT_0173_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20_00sec_-15_00C_LIGHT_0174_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20_00sec_-14_90C_LIGHT_0173_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 22.3129* 11 32 02.59 +15 52 43.8 13.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1132030+155244,2461121.8129,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1132030+155244 20260322.3129 13.74CV 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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:32:02.59 +15:52:43.8 ;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-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20_00sec_-15_00C_LIGHT_0174_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20_00sec_-14_90C_LIGHT_0173_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20_00sec_-15_00C_LIGHT_0174_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20_00sec_-15_00C_LIGHT_0407_fits__*pix.png resample_wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20_00sec_-14_90C_LIGHT_0173_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.87513731 11.02.2026 09:00:01.864 /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
First image: 2461082.87513731 11.02.2026 09:00:01.864 /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
Last image: 2461121.81314587 22.03.2026 07:30:45.803 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
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): 6159
Objects passed selection criteria: 6146
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 5489.75
Average stars matched: 4989 (90.8785 %)
Memory usage VmPeak: 112048 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 02:33:03 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: 2461082.87513731 11.02.2026 09:00:01.864 /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
First image: 2461082.87513731 11.02.2026 09:00:01.864 /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
Last image: 2461121.81314587 22.03.2026 07:30:45.803 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 88
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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): 29599
Objects passed selection criteria: 29528
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: 28459.5
Average stars matched: 26281.8 (92.3479 %)
Memory usage VmPeak: 131912 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 02:33:45 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/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
SExtractor catalog cache: saved Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat to cache
SExtractor catalog cache: saved Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.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: 2461121.81261001
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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits exists and is non-empty
Saving wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits to local_wcs_cache/
'wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits' -> 'local_wcs_cache/wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits'
wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits exists and is non-empty
Saving wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits to local_wcs_cache/
'wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits' -> 'local_wcs_cache/wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits'
wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits exists and is non-empty
Saving wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits to local_wcs_cache/
'wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits' -> 'local_wcs_cache/wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits'
wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits exists and is non-empty
Saving wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits to local_wcs_cache/
'wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits' -> 'local_wcs_cache/wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.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 11:33:20.255 +13:59:50.78
Second-epoch image center 11:33:33.886 +14:00:50.65
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:33:20.255 +13:59:50.78
Second-epoch image center 11:33:31.471 +14:01:19.92
Angular distance between the image centers 0.05 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 11:33:33.886 +14:00:50.65
Second-epoch second image center 11:33:31.471 +14:01:19.92
Angular distance between the image centers 0.01270 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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits &> /tmp/tmp.QCgnWEEcQE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits &> /tmp/tmp.fmVem30Aw1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits &> /tmp/tmp.nIFyohUASA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits &> /tmp/tmp.ToPipE7zYA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits and wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits and wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat
Found non-empty wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits and wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat
The reference image (wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits) and catalog (wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat) found
'wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.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 3060 out of 4694 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.747371
a=0.000000 b=1.000000 c=22.747371
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.07
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
2.1 pix Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
2.2 pix fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
2.1 pix fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
Limiting magnitude estimates:
15.1 mag. Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
15.0 mag. Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
15.5 mag. fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
15.5 mag. fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.QCgnWEEcQE (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits' -> 'wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
WCS_IMAGE_NAME=wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
WCS-calibrated image found: wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
Checking if the catalog wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat corresponding to the image wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits alredy exist and is non-empty...
Catalog wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat corresponding to the image wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
WCS catalog name: wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=329, passed=4694
Got 4694 stars (including 4360 good ones) from the SExtractor catalog wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat
util/solve_plate_with_UCAC5 got 4694 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 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits -region wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fmVem30Aw1 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.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-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits' -> 'wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
WCS_IMAGE_NAME=wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
WCS-calibrated image found: wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
Checking if the catalog wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits.cat corresponding to the image wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits alredy exist and is non-empty...
Catalog wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits.cat corresponding to the image wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
WCS catalog name: wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=328, passed=4572
Got 4572 stars (including 4242 good ones) from the SExtractor catalog wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits.cat
util/solve_plate_with_UCAC5 got 4572 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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits -region wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.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.nIFyohUASA (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_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.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_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
WCS-calibrated image found: wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
Checking if the catalog wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits.cat corresponding to the image wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits.cat corresponding to the image wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
WCS catalog name: wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=396, passed=6456
Got 6456 stars (including 6053 good ones) from the SExtractor catalog wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits.cat
util/solve_plate_with_UCAC5 got 6456 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 976 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: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.23"
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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.23"
Estimated accuracy of the plate solution: 0.22"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits -region wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.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.ToPipE7zYA (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_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.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_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
WCS-calibrated image found: wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
Checking if the catalog wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
WCS catalog name: wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=399, passed=6397
Got 6397 stars (including 5988 good ones) from the SExtractor catalog wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits.cat
util/solve_plate_with_UCAC5 got 6397 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 975 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: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.24"
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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.24"
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits -region wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits'
Saving fully-calibrated image wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits'
Saving fully-calibrated image wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits'
Saving fully-calibrated image wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits'
Preparing the HTML report for the field Leo-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20186.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20186_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 20186_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:02:18.05 +16:30:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 2.101 3969885761146749952 165.57507332365 +16.50856920825 10.7417 9.7194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.101#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: 1s
Prepared the HTML report for the field Leo-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
SExtractor catalog cache: saved Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat to cache
SExtractor catalog cache: saved Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
Creating symlink local_wcs_cache/wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits exists and is non-empty
wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits exists and is non-empty
wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits exists and is non-empty
wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.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 11:33:20.255 +13:59:50.78
Second-epoch image center 11:33:33.886 +14:00:50.65
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:33:20.255 +13:59:50.78
Second-epoch image center 11:33:31.471 +14:01:19.92
Angular distance between the image centers 0.05 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 11:33:33.886 +14:00:50.65
Second-epoch second image center 11:33:31.471 +14:01:19.92
Angular distance between the image centers 0.01270 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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits &> /tmp/tmp.sAwBMrHuJc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits &> /tmp/tmp.nrX9qqCFYV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits &> /tmp/tmp.r0n0Qynoli
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits &> /tmp/tmp.8VmAcneSXQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits and wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits and wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat
Found non-empty wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits and wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat
The reference image (wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits) and catalog (wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat) found
'wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.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 3186 out of 26073 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.624625
a=0.000000 b=1.000000 c=22.624625
From vast_summary.log: estimated ref. image limiting mag.: -7.42
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 77 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
2.0 pix Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
2.1 pix fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
2.1 pix fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
Limiting magnitude estimates:
15.2 mag. Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
15.2 mag. Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
15.6 mag. fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
15.6 mag. fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
All-image limiting magnitude estimate: 15.6 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.sAwBMrHuJc (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits' -> 'wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
WCS_IMAGE_NAME=wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
WCS-calibrated image found: wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
Checking if the catalog wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat corresponding to the image wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits alredy exist and is non-empty...
Catalog wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat corresponding to the image wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
WCS catalog name: wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=925, passed=26052
Got 26052 stars (including 25073 good ones) from the SExtractor catalog wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat
util/solve_plate_with_UCAC5 got 26052 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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits -region wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nrX9qqCFYV (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.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-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits' -> 'wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
WCS_IMAGE_NAME=wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
WCS-calibrated image found: wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
Checking if the catalog wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits.cat corresponding to the image wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits alredy exist and is non-empty...
Catalog wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits.cat corresponding to the image wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
WCS catalog name: wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=880, passed=25436
Got 25436 stars (including 24500 good ones) from the SExtractor catalog wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits.cat
util/solve_plate_with_UCAC5 got 25436 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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits -region wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.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.r0n0Qynoli (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_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.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_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
WCS-calibrated image found: wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
Checking if the catalog wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits.cat corresponding to the image wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits.cat corresponding to the image wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
WCS catalog name: wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1129, passed=31424
Got 31424 stars (including 30241 good ones) from the SExtractor catalog wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits.cat
util/solve_plate_with_UCAC5 got 31424 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 976 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: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.25"
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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.24"
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits -region wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.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.8VmAcneSXQ (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_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.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_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
WCS-calibrated image found: wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
Checking if the catalog wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
WCS catalog name: wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1137, passed=31716
Got 31716 stars (including 30520 good ones) from the SExtractor catalog wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits.cat
util/solve_plate_with_UCAC5 got 31716 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 976 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: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.25"
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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.25"
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits -region wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.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-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/wcs_Leo-06-Q1b1x1_2026-02-11_03-00-01_20.00sec_-15.00C_LIGHT_0407.fits
Saving fully-calibrated image wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.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_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/wcs_Leo-06-Q1b1x1_2026-02-11_03-00-40_20.00sec_-15.00C_LIGHT_0408.fits
Saving fully-calibrated image wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.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_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-29-59_20.00sec_-14.90C_LIGHT_0173.fits
Saving fully-calibrated image wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.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_2026-03-22_CI_Leo-06-Q1b1x1_023126_TTUQ1b1x1_8002_LlPScVWN/wcs_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174.fits
Preparing the HTML report for the field Leo-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out31568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31941.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32038.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32098.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32114.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out31919.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out31981.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out31987.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out32033.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out32059.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out32069.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out08112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31982.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
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: 4s
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Considering the candidate 31567_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31567_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:04:00.87 +15:08:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31568_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31568_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:41:25.78 +19:05:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 1.020 3975657406918664448 175.35711715083 +19.08901184571 14.7534 14.2306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31579_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31579_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:25:36.49 +16:28:18.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31622_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
Preparing report for the candidate 31622_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
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Considering the candidate 31624_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
Preparing report for the candidate 31624_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
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Considering the candidate 31783_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31783_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:08:39.36 +12:17:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31803_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
Preparing report for the candidate 31803_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
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Considering the candidate 31822_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31822_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:03:01.90 +12:37:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31848_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31848_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 12:02:59.16 +12:48:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 4.783 3919965081387956352 180.74786244776 +12.81060180636 14.6124 14.1490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31849_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31849_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 12:02:54.64 +18:45:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31893_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31893_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:11:43.51 +17:06:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31901_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31901_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:05:19.48 +18:05:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.023 3983648794868003072 166.33124493330 +18.08832984335 14.6330 14.0313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31919_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31919_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 12:03:59.45 +09:12:59.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.59, MAG_FAINT_SEARCH_LIMIT=15.57)
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Considering the candidate 31923_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
Preparing report for the candidate 31923_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
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Considering the candidate 31925_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31925_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:25:51.07 +18:50:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 3.214 3977183322899703168 171.46362236006 +18.84168821303 14.7664 14.2180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31926_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31926_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:09:19.65 +09:01:17.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)
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Considering the candidate 31929_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31929_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:07:02.91 +12:09:44.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31930_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31930_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:27:56.32 +12:00:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31931_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31931_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 12:00:00.79 +17:29:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31940_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31940_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:08:48.55 +09:11:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.55, MAG_FAINT_SEARCH_LIMIT=15.53)GAIADR2_OUTPUT=# 0.694 3867026998124154880 167.20227345888 +09.19083575575 14.6556 14.0792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31941_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31941_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:02:14.92 +14:28:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 0.871 3968993576180182912 165.56240197631 +14.46989121070 14.5852 14.0816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31944_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31944_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:11:18.05 +11:33:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31947_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31947_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:15:57.47 +13:20:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31950_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
Preparing report for the candidate 31950_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
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Considering the candidate 31951_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31951_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:03:00.29 +11:26:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)GAIADR2_OUTPUT=# 1.937 3868537177344885120 165.75089929490 +11.43783317248 14.6823 14.1595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31952_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31952_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:04:30.17 +13:17:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 0.786 3967906777655772544 166.12591992463 +13.29159452258 14.5979 14.0669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31957_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31957_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:07:46.49 +12:32:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)GAIADR2_OUTPUT=# 0.902 3964793957158349184 166.94367030269 +12.54966883896 14.3727 13.6113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.902#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31963_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31963_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:05:36.67 +15:28:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 0.945 3969526461362666240 166.40303693471 +15.48224724934 14.4474 13.6850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31967_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31967_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:02:52.29 +10:27:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 0.711 3868153894463302016 165.71782232788 +10.45211498308 14.6913 14.1607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31969_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31969_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:26:09.34 +11:17:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31979_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31979_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:35:19.88 +12:39:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)GAIADR2_OUTPUT=# 1.711 3917663356873996288 173.83332040860 +12.66044570311 14.0957 13.0186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31981_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31981_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:09:52.37 +09:31:11.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.59, MAG_FAINT_SEARCH_LIMIT=15.57)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31982_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
Preparing report for the candidate 31982_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31984_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31984_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:08:42.71 +10:01:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)GAIADR2_OUTPUT=# 1.536 3867351732011523072 167.17831705908 +10.03090610885 14.6704 14.1752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31987_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31987_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:45:48.52 +10:28:37.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31993_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31993_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:24:17.42 +09:27:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.411 3914935880842451072 171.07225660680 +09.46052844226 14.5328 13.6608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31994_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31994_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:11:44.75 +16:19:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 4.574 3971096387875702144 167.93698618033 +16.32469297024 14.6287 13.3965 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31995_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31995_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:09:13.15 +12:02:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 1.399 3964622192826326784 167.30504769815 +12.03385268290 14.9876 14.4983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31998_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 31998_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:10:01.24 +09:54:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 1.476 3867339362505742336 167.50557642790 +09.90090101320 14.6339 14.1226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32006_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32006_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:16:58.40 +10:35:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32019_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32019_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:04:20.08 +12:59:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 1.332 3967793356159390464 166.08355369546 +12.99951976838 14.8275 14.3568 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32021_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32021_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:09:11.91 +14:35:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 0.569 3968658053335264512 167.29970121799 +14.59219530893 14.4888 14.0506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32029_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32029_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:12:22.37 +18:26:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32032_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32032_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:59:34.66 +12:57:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 0.234 3919947798439591552 179.89443720211 +12.96610484215 14.7591 14.0226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32033_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32033_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:06:51.20 +14:12:11.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32034_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32034_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:06:53.87 +12:32:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 1.688 3964711248972994816 166.72482146964 +12.53510966656 14.7428 14.2235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32035_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32035_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:04:52.35 +09:06:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.440 3866828669418737792 166.21785182546 +09.10571209039 14.7422 14.2118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32037_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32037_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:05:12.69 +11:07:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 0.569 3868486565450289280 166.30299379175 +11.12797644790 14.5896 13.9822 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32038_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32038_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:59:58.44 +17:55:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 0.531 3926707939524675712 179.99362196335 +17.92096473117 14.6992 14.1117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32039_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32039_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:08:42.36 +18:24:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 0.567 3984014623002400128 167.17662133120 +18.41330920406 14.8556 14.3766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32042_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32042_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:53:05.92 +09:27:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.954 3912259669540649472 178.27455951629 +09.46168741713 14.7647 14.1791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32046_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32046_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:09:59.85 +12:56:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 0.717 3964835257563845120 167.49944789916 +12.94268605042 14.7209 14.0985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32047_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32047_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:15:13.96 +12:54:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 1.022 3964975617095084032 168.80843306102 +12.90328158955 13.8094 12.5793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32050_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32050_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:05:13.86 +16:32:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)GAIADR2_OUTPUT=# 1.063 3969850744278041856 166.30754449770 +16.53686337222 14.6925 14.1364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32052_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32052_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:08:01.12 +17:49:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 1.091 3971575465705400960 167.00491800636 +17.82648082467 14.6259 14.0675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32055_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32055_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:06:43.37 +10:30:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 2.017 3868184474630632704 166.68104078568 +10.50035036107 14.8559 14.2322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32059_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32059_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:53:58.63 +09:37:38.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)
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Considering the candidate 32065_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32065_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:09:03.28 +17:59:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.243 3971607527636278912 167.26373152591 +17.98424370410 14.7967 14.4128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32067_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32067_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:05:51.19 +11:57:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 0.708 3964655865369917824 166.46348717386 +11.96537912762 14.6979 13.9099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32069_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32069_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:22:04.69 +19:03:01.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)
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Considering the candidate 32071_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32071_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:07:09.24 +17:21:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 0.651 3971452737015029632 166.78857057391 +17.35383210302 14.6756 14.1971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.651#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32073_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32073_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:08:44.57 +10:40:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 2.063 3868213989645901568 167.18625102508 +10.68329338218 14.8137 14.2337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32079_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32079_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:08:40.45 +09:33:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 1.297 3867230545214305280 167.16866753253 +09.55621732143 14.5311 13.9078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32083_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32083_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:34:36.30 +09:41:05.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)
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Considering the candidate 32087_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32087_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:03:30.99 +18:52:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 0.759 3983939272096219392 165.87901441740 +18.87898862748 14.6815 13.9234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32088_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32088_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:02:57.91 +10:16:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 1.813 3868116231894898304 165.74180333327 +10.28207840868 14.7602 14.3018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32091_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32091_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:06:43.52 +13:44:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 1.470 3967950723761132288 166.68175200677 +13.74902033319 14.6146 13.8802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32093_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32093_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:12:37.46 +16:17:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 0.809 3970437887782654080 168.15627943823 +16.29851162312 14.9127 14.2731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32096_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32096_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:04:49.29 +09:00:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 1.175 3866819156066781568 166.20557362974 +09.01170529754 14.8714 14.3503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32098_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32098_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:23:43.31 +10:08:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 1.068 3915409358036965760 170.93067089740 +10.14476576607 15.1788 14.2933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32099_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32099_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:04:13.55 +15:06:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 4.962 3969418228186734336 166.05724680536 +15.10385104123 15.1898 14.6546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.962#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32101_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32101_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:22:51.54 +09:46:04.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)
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Considering the candidate 32114_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32114_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:02:37.47 +10:24:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)GAIADR2_OUTPUT=# 0.602 3868130220603568768 165.65628417106 +10.40997522774 14.4817 13.9740 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32121_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32121_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:05:10.14 +11:53:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 0.478 3964652017079227264 166.29237850751 +11.88345959312 14.7195 14.0765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32126_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32126_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks
**** FOUND 11:07:22.52 +09:21:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 1.509 3867200720961411456 166.84425321125 +09.35218635141 14.4687 13.9590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32128_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174
The candidate 32128_fd_Leo-06-Q1b1x1_2026-03-22_02-30-45_20.00sec_-15.00C_LIGHT_0174 did not pass the final checks