This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3624* 11 22 42.28 +02 22 18.6 10.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8624,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3624 10.93CV 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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:22:42.28 +02:22:18.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3624* 11 38 26.69 +03 22 05.4 11.7 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
QZ Vir,2461118.8624,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
QZ Vir 20260319.3624 11.71CV 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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:26.69 +03:22:05.4 ;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-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3624* 10 53 30.88 +08 43 35.3 11.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8624,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3624 11.94CV 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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:53:30.88 +08:43:35.3 ;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-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3624* 11 10 21.69 +01 07 55.4 12.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8624,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3624 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:10:21.69 +01:07:55.4 ;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-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3624* 10 49 14.76 +02 22 12.6 12.7 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8624,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3624 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:49:14.76 +02:22:12.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3624* 11 20 29.23 +08 50 45.5 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,2461118.8624,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3624 12.82CV 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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:20:29.23 +08:50:45.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3624* 11 21 42.64 +07 22 55.5 13.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8624,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3624 13.32CV 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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:21:42.64 +07:22:55.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3624* 11 21 46.53 +09 21 50.3 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,2461118.8624,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3624 14.09CV 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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:21:46.53 +09:21:50.3 ;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-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3624* 11 22 36.99 +08 18 45.0 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,2461118.8624,14.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3624 14.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:22:36.99 +08:18:45.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3624* 10 51 00.28 +08 26 12.8 14.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8624,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3624 14.48CV 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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:51:00.28 +08:26:12.8 ;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-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3624* 10 59 40.41 +06 37 30.7 13.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HQ Leo,2461118.8624,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HQ Leo 20260319.3624 13.19CV 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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:59:40.41 +06:37:30.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20_00sec_-15_00C_LIGHT_0103_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20_00sec_-14_90C_LIGHT_0102_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: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
First image: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Last image: 2461118.86270448 19.03.2026 08:42:07.667 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
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: 2 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): 6124
Objects passed selection criteria: 6124
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: 5817.5
Average stars matched: 5566.75 (95.6897 %)
Memory usage VmPeak: 112168 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 04:01:58 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: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
First image: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Last image: 2461118.86270448 19.03.2026 08:42:07.667 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 283
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: 9 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): 31984
Objects passed selection criteria: 31897
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: 30416.8
Average stars matched: 29200.5 (96.0014 %)
Memory usage VmPeak: 133312 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 04:02:43 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
SExtractor catalog cache: saved Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461118.86217911
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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits exists and is non-empty
Saving wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits to local_wcs_cache/
'wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'local_wcs_cache/wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits exists and is non-empty
Saving wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits to local_wcs_cache/
'wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'local_wcs_cache/wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits exists and is non-empty
Saving wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits'
wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits exists and is non-empty
Saving wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:54.845 +05:57:56.20
Angular distance between the image centers 0.18 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:55.446 +05:58:11.42
Angular distance between the image centers 0.19 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:54.845 +05:57:56.20
Second-epoch second image center 11:08:55.446 +05:58:11.42
Angular distance between the image centers 0.00491 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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits &> /tmp/tmp.dBQxVQNgEK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits &> /tmp/tmp.xjslT0XRfy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits &> /tmp/tmp.cuOKw4OAxI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits &> /tmp/tmp.AefwQ6RlEd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
Found non-empty wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
The reference image (wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits) and catalog (wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat) found
'wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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 3354 out of 5629 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.832371
a=0.000000 b=1.000000 c=22.832371
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.15
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
2.1 pix Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
2.4 pix fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
2.4 pix fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
Limiting magnitude estimates:
15.2 mag. Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
15.2 mag. Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
15.2 mag. fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
15.2 mag. fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.dBQxVQNgEK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS-calibrated image found: wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Checking if the catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS catalog name: wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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=5629
Got 5629 stars (including 5225 good ones) from the SExtractor catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
util/solve_plate_with_UCAC5 got 5629 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 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 - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits -region wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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.xjslT0XRfy (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS-calibrated image found: wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Checking if the catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS catalog name: wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=431, passed=5671
Got 5671 stars (including 5234 good ones) from the SExtractor catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
util/solve_plate_with_UCAC5 got 5671 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.3'
Seting catalog search parameters based on the expected field of view 944.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013115 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010492 (37.8 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 883 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: 2.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.46"
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 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.26"
Estimated accuracy of the plate solution: 1.14"
Excluding outliers - 920 stars left (next iteration limit 970)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits -region wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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.cuOKw4OAxI (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
Checking if the catalog wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
WCS catalog name: wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=381, passed=6102
Got 6102 stars (including 5714 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits.cat
util/solve_plate_with_UCAC5 got 6102 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits -region wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.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.AefwQ6RlEd (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
Checking if the catalog wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
WCS catalog name: wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=380, passed=6042
Got 6042 stars (including 5654 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits.cat
util/solve_plate_with_UCAC5 got 6042 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits -region wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
Saving fully-calibrated image wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
Saving fully-calibrated image wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits'
Saving fully-calibrated image wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits'
Preparing the HTML report for the field Leo-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20371.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20329_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
Preparing report for the candidate 20329_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20354_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
Preparing report for the candidate 20354_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20361_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
Preparing report for the candidate 20361_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20371_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
Preparing report for the candidate 20371_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20372_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 20372_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 11:23:23.28 +06:07:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.543 3814378052059528320 170.84688644954 +06.12037222420 11.9500 11.4330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20377_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 20377_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 11:03:12.02 +07:11:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20378_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 20378_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 11:23:55.31 +10:18:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.612 3915600771844146816 170.98031518049 +10.31634927563 12.4610 12.1186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Leo-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:22:42.28 +02:22:18.6
11:38:26.69 +03:22:05.4
10:53:30.88 +08:43:35.3
11:10:21.69 +01:07:55.4
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
SExtractor catalog cache: saved Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Creating symlink local_wcs_cache/wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits exists and is non-empty
wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits exists and is non-empty
wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits exists and is non-empty
wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:54.845 +05:57:56.20
Angular distance between the image centers 0.18 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:55.446 +05:58:11.42
Angular distance between the image centers 0.19 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:54.845 +05:57:56.20
Second-epoch second image center 11:08:55.446 +05:58:11.42
Angular distance between the image centers 0.00491 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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits &> /tmp/tmp.OGtAqI0lwK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits &> /tmp/tmp.FXYHPreWps
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits &> /tmp/tmp.w8U40cQD4I
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits &> /tmp/tmp.KYheMDDYot
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
Found non-empty wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
The reference image (wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits) and catalog (wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat) found
'wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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 3441 out of 31032 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.714936
a=0.000000 b=1.000000 c=22.714936
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 173 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
2.0 pix Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
2.3 pix fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
2.2 pix fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
Limiting magnitude estimates:
15.3 mag. Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
15.3 mag. Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
15.3 mag. fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
15.3 mag. fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.OGtAqI0lwK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS-calibrated image found: wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Checking if the catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS catalog name: wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1190, passed=31016
Got 31016 stars (including 29781 good ones) from the SExtractor catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
util/solve_plate_with_UCAC5 got 31016 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 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 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 - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits -region wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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.FXYHPreWps (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS-calibrated image found: wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Checking if the catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS catalog name: wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1251, passed=31400
Got 31400 stars (including 30103 good ones) from the SExtractor catalog wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
util/solve_plate_with_UCAC5 got 31400 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.3'
Seting catalog search parameters based on the expected field of view 944.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013115 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010492 (37.8 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 886 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: 2.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.38"
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 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.33"
Estimated accuracy of the plate solution: 1.09"
Excluding outliers - 918 stars left (next iteration limit 973)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits -region wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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.w8U40cQD4I (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
Checking if the catalog wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
WCS catalog name: wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1201, passed=29976
Got 29976 stars (including 28731 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits.cat
util/solve_plate_with_UCAC5 got 29976 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits -region wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.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.KYheMDDYot (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
Checking if the catalog wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits.cat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
WCS catalog name: wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1218, passed=30171
Got 30171 stars (including 28917 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits.cat
util/solve_plate_with_UCAC5 got 30171 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits -region wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.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-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/wcs_Leo-07-Q2b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Saving fully-calibrated image wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/wcs_Leo-07-Q2b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Saving fully-calibrated image wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-41-22_20.00sec_-14.90C_LIGHT_0102.fits
Saving fully-calibrated image wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-07-Q2b1x1_035948_TTUQ2b1x1_8914_Nyyy97I3/wcs_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103.fits
Preparing the HTML report for the field Leo-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52704.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out12912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52758.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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 52330_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52330_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 52334_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52334_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 11:12:54.04 +01:51:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 0.700 3810562570616580480 168.22499818756 +01.86268049052 13.9506 13.4977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52335_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52335_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52337_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52337_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 11:03:50.52 +05:56:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 0.743 3816378059414569344 165.96030960471 +05.93347379355 14.0379 13.5089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52344_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52344_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 11:35:21.11 +01:09:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52345_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52345_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 10:40:19.17 +10:35:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.942 3870412252691812864 160.08037331558 +10.59505176164 12.3431 11.8805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.942#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52370_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52370_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 11:22:42.27 +02:22:18.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52381_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52381_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 10:38:38.39 +10:59:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 1.836 3870672149752805120 159.66043997366 +10.99169785459 11.2718 10.7728 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52398_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52398_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 11:38:26.70 +03:22:05.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52399_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52399_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52404_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52404_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 10:53:30.88 +08:43:35.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52411_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52411_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52414_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52414_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 52417_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52417_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 11:10:21.68 +01:07:55.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52423_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52423_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52429_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52429_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52438_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52438_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52441_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52441_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52444_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52444_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 10:42:39.12 +03:33:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52456_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
Preparing report for the candidate 52456_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
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Considering the candidate 52462_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52462_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52465_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
Preparing report for the candidate 52465_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
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Considering the candidate 52466_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52466_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52476_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52476_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 10:51:21.81 +02:00:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.608 3808319742990503680 162.84077167712 +02.00408873428 13.0845 12.4899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52481_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52481_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52484_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52484_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52485_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52485_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52486_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52486_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52488_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52488_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52490_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52490_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52492_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52492_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 52495_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52495_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52504_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52504_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52507_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52507_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52510_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52510_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52512_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52512_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52522_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52522_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52524_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52524_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52525_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52525_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52526_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52526_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52527_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52527_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52529_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52529_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52530_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52530_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52531_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52531_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52532_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
Preparing report for the candidate 52532_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52535_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52535_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52541_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52541_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52543_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52543_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52544_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52544_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52545_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52545_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52546_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52546_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52548_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52548_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52549_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52549_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52550_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52550_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52552_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52552_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52559_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52559_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52560_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52560_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52564_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52564_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52567_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52567_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 11:04:58.20 +07:22:12.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52568_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52568_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52569_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52569_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52571_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52571_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52573_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52573_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52574_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52574_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52581_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52581_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52584_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52584_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52585_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52585_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52589_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52589_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52592_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52592_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52595_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52595_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52596_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52596_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 52598_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52598_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52599_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52599_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52600_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52600_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52605_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52605_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 52607_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52607_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52608_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52608_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52610_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52610_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52611_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52611_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52613_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52613_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52615_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52615_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 10:48:17.04 +02:47:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.257 3809378538327949056 162.07079612601 +02.79396644329 13.9554 13.4867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52616_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52616_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52619_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52619_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52623_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52623_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52625_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52625_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52626_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52626_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 52627_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52627_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52628_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52628_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52631_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52631_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 52632_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52632_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52634_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52634_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 52637_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52637_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52638_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52638_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 10:38:36.71 +11:03:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 0.171 3870675521302444032 159.65299222069 +11.05227177888 13.7624 13.3199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52639_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52639_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52640_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52640_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52642_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52642_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52644_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52644_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52655_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52655_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52656_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52656_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52660_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52660_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52661_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52661_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52663_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52663_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52667_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52667_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52671_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52671_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52673_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52673_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52674_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52674_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52678_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
Preparing report for the candidate 52678_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
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Considering the candidate 52680_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52680_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52682_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52682_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52688_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52688_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52689_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52689_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52692_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52692_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 10:38:46.22 +10:56:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.582 3870670573500120064 159.69242455586 +10.93379296057 14.0990 13.6565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52693_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52693_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52694_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52694_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52698_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52698_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52701_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52701_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52702_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52702_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52704_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52704_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 10:38:25.21 +10:22:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 2.527 3870569074833013760 159.60574307590 +10.36945412425 13.9357 13.4389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52705_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52705_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52706_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52706_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52707_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52707_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52708_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52708_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52711_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52711_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 10:39:54.96 +10:35:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 2.737 3870599277043029376 159.97972508892 +10.59795758082 13.7251 13.2054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52713_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52713_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52716_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52716_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52724_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52724_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52729_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52729_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52733_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52733_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 52736_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
Preparing report for the candidate 52736_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
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Considering the candidate 52739_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52739_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52740_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52740_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 52742_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52742_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 52745_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52745_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52748_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52748_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
**** FOUND 10:47:58.36 +06:54:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 1.347 3865332616346531840 161.99311857828 +06.90428783035 14.2970 13.7970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52754_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52754_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52757_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52757_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 52758_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
Preparing report for the candidate 52758_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
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Considering the candidate 52760_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52760_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 52761_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52761_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52764_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52764_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52769_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52769_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52775_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52775_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52780_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52780_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 52784_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52784_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52786_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52786_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52793_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52793_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 52798_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52798_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 52800_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52800_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 52802_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52802_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 52805_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52805_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52807_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52807_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52818_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52818_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 52822_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52822_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 52834_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52834_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 52837_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52837_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 52849_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52849_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52851_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52851_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 52856_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52856_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 52859_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52859_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52864_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52864_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 52865_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52865_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 52867_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52867_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52868_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52868_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52877_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52877_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52878_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52878_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52885_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52885_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52890_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52890_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52894_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52894_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52899_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52899_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52901_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52901_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52916_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 52916_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15713_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103
The candidate 15713_fd_Leo-07-Q2b1x1_2026-03-19_03-42-07_20.00sec_-15.00C_LIGHT_0103 did not pass the final checks