This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 11 20 08.85 +02 40 25.9 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,2461121.8005,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3005 10.88CV 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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:20:08.85 +02:40:25.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 11 07 33.95 +01 27 09.7 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,2461121.8005,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3005 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:07:33.95 +01:27:09.7 ;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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 10 51 04.97 +08 47 55.9 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,2461121.8005,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3005 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:51:04.97 +08:47:55.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 11 37 46.12 +05 23 26.6 12.5 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.8005,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3005 12.49CV 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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:37:46.12 +05:23:26.6 ;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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 11 18 05.18 +09 06 11.9 12.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.8005,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3005 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:18:05.18 +09:06:11.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 10 46 57.60 +02 50 40.7 13.1 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,2461121.8005,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3005 13.08CV 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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:46:57.60 +02:50:40.7 ;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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 11 19 36.15 +07 35 27.7 13.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.8005,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3005 13.43CV 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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:19:36.15 +07:35:27.7 ;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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 11 38 26.74 +03 22 06.1 14.1 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,2461121.8005,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
QZ Vir 20260322.3005 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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:26.74 +03:22:06.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 11 19 31.46 +09 35 22.7 14.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.8005,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3005 14.21CV 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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:19:31.46 +09:35:22.7 ;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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 11 20 04.62 +08 37 17.5 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,2461121.8005,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3005 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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:20:04.62 +08:37:17.5 ;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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 11 14 57.61 +07 07 50.4 14.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.8005,14.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3005 14.55CV 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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:14:57.61 +07:07:50.4 ;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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 11 38 33.60 +06 56 44.5 14.7 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
target,2461121.8005,14.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.3005 14.73CV 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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:38:33.60 +06:56:44.5 ;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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 11 07 55.61 +08 44 54.3 14.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.8005,14.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3005 14.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:07:55.61 +08:44:54.3 ;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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.3005 2461121.8005 14.76 11:13:52.88 +04:17:28.3
253.09605 57.39593 galactic Leo Second-epoch detections are separated by 1.2" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 11:13:52.88 +04:17:28.3 (user input) | T | P | (position from user input) J-Ks=13.473+/- (unrealisitic color!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 11 13 52.88 +04 17 28.3 14.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.8005,14.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.3005 14.76CV 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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:13:52.88 +04:17:28.3 ;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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 11 18 13.70 +06 05 53.5 14.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.8005,14.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3005 14.69CV 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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:18:13.70 +06:05:53.5 ;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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.3005 2461121.8005 14.87 11:25:17.09 +02:26:53.8
259.37449 57.84003 galactic Leo Second-epoch detections are separated by 2.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J171.3214+02.4468 | 11:25:17.09 +02:26:53.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 11 25 17.09 +02 26 53.8 14.9 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
ATO J171.3214+02.4468,2461121.8005,14.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J171.3214+02.4468 20260322.3005 14.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:25:17.09 +02:26:53.8 ;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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.3006* 10 50 17.98 +09 54 19.4 14.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.8005,14.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.3005 14.66CV 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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:50:17.98 +09:54:19.4 ;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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20_00sec_-14_90C_LIGHT_0158_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20_00sec_-14_90C_LIGHT_0423_fits__*pix.png resample_wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20_00sec_-14_90C_LIGHT_0157_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Last image: 2461121.80099625 22.03.2026 07:13:16.076 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
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: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6520
Objects passed selection criteria: 6513
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: 6178.25
Average stars matched: 5792.25 (93.7523 %)
Memory usage VmPeak: 112504 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 02:17:16 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-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Last image: 2461121.80099625 22.03.2026 07:13:16.076 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 68
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: 16 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): 33247
Objects passed selection criteria: 33179
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 32489
Average stars matched: 30612.2 (94.2234 %)
Memory usage VmPeak: 135120 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 02:18:25 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461121.80009630
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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits exists and is non-empty
Saving wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits to local_wcs_cache/
'wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits exists and is non-empty
Saving wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits to local_wcs_cache/
'wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits exists and is non-empty
Saving wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits'
wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits exists and is non-empty
Saving wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.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 11:08:30.999 +05:59:57.60
Angular distance between the image centers 0.08 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:33.723 +06:00:23.08
Angular distance between the image centers 0.09 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:30.999 +05:59:57.60
Second-epoch second image center 11:08:33.723 +06:00:23.08
Angular distance between the image centers 0.01332 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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits &> /tmp/tmp.Na2oINrnRR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_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-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits &> /tmp/tmp.GRwPiF53Bj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_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_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits &> /tmp/tmp.VvzSYQ1ucT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits &> /tmp/tmp.FuCcS3kNNJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
Found non-empty wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
The reference image (wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits) and catalog (wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat) found
'wcs_Leo-07-Q1b1x1_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 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
2.1 pix Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
2.2 pix fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
2.1 pix fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
Limiting magnitude estimates:
15.2 mag. Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
15.2 mag. Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
15.4 mag. fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
15.4 mag. fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
All-image limiting magnitude estimate: 15.4 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Na2oINrnRR (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'wcs_Leo-07-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits -region wcs_Leo-07-Q1b1x1_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-Q1b1x1_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.GRwPiF53Bj (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'wcs_Leo-07-Q1b1x1_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-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits -region wcs_Leo-07-Q1b1x1_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-Q1b1x1_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.VvzSYQ1ucT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=417, passed=6846
Got 6846 stars (including 6419 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits.cat
util/solve_plate_with_UCAC5 got 6846 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.26"
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-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits -region wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.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.FuCcS3kNNJ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=441, passed=6737
Got 6737 stars (including 6290 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits.cat
util/solve_plate_with_UCAC5 got 6737 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
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: 0.28"
Estimated accuracy of the plate solution: 0.26"
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-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits -region wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.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-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
Saving fully-calibrated image wcs_Leo-07-Q1b1x1_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-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits'
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits'
Preparing the HTML report for the field Leo-07-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20335.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20311_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 20311_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20332_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 20332_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20333_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 20333_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:23:23.27 +06:07:13.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20335_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 20335_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20340_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 20340_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:12:36.11 +06:23:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.524 3817216510045895168 168.15032279470 +06.39169460111 11.8878 11.0081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20341_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 20341_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:03:12.07 +07:11:09.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Leo-07-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:20:08.85 +02:40:25.9
11:07:33.95 +01:27:09.7
10:51:04.97 +08:47:55.9
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Creating symlink local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits exists and is non-empty
wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits exists and is non-empty
wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits exists and is non-empty
wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.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 11:08:30.999 +05:59:57.60
Angular distance between the image centers 0.08 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:33.723 +06:00:23.08
Angular distance between the image centers 0.09 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:30.999 +05:59:57.60
Second-epoch second image center 11:08:33.723 +06:00:23.08
Angular distance between the image centers 0.01332 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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits &> /tmp/tmp.2v6AdHc3Kg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_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-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits &> /tmp/tmp.nTML23Pebg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_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_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits &> /tmp/tmp.FNFnsCYUJx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits &> /tmp/tmp.yZLXkawLTD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
Found non-empty wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
The reference image (wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits) and catalog (wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat) found
'wcs_Leo-07-Q1b1x1_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 63 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
2.0 pix Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
2.2 pix fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
2.1 pix fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
Limiting magnitude estimates:
15.3 mag. Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
15.3 mag. Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
15.5 mag. fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
15.5 mag. fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.2v6AdHc3Kg (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'wcs_Leo-07-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits -region wcs_Leo-07-Q1b1x1_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-Q1b1x1_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.nTML23Pebg (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'wcs_Leo-07-Q1b1x1_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-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits -region wcs_Leo-07-Q1b1x1_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-Q1b1x1_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.FNFnsCYUJx (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1267, passed=33878
Got 33878 stars (including 32558 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits.cat
util/solve_plate_with_UCAC5 got 33878 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.25"
Estimated accuracy of the plate solution: 0.23"
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-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits -region wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.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.yZLXkawLTD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1276, passed=34482
Got 34482 stars (including 33142 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits.cat
util/solve_plate_with_UCAC5 got 34482 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 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-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits -region wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.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-Q1b1x1_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_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Saving fully-calibrated image wcs_Leo-07-Q1b1x1_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_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-11-58_20.00sec_-14.90C_LIGHT_0157.fits
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-07-Q1b1x1_021356_TTUQ1b1x1_10136_ztuaVWd9/wcs_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158.fits
Preparing the HTML report for the field Leo-07-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52905.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out52685.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out52823.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out52849.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out52858.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out52867.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out52383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52809.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 22s
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: 10s
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Considering the candidate 52341_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52341_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:20:08.84 +02:40:25.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52366_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52366_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:07:33.92 +01:27:09.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52367_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52367_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:51:04.95 +08:47:55.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52383_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 52383_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
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Considering the candidate 52399_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52399_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:40:59.66 +05:47:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52410_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 52410_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
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Considering the candidate 52432_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 52432_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
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Considering the candidate 52457_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 52457_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
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Considering the candidate 52527_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52527_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:31:39.68 +03:01:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52566_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 52566_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
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Considering the candidate 52588_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 52588_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
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Considering the candidate 52589_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52589_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:03:50.55 +05:56:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52618_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52618_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:32:23.78 +10:27:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.266 3914729207016269824 173.09908316451 +10.46345378432 14.6792 14.3201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52642_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52642_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:36:11.75 +03:19:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 2.507 3800791970990787072 174.04831760366 +03.32116403505 14.9009 14.3989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52655_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 52655_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
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Considering the candidate 52667_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52667_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:16:58.60 +10:35:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52685_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52685_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:28:13.22 +09:03:42.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)
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Considering the candidate 52694_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52694_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:09:15.44 +04:41:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52695_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52695_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:50:01.14 +06:32:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)GAIADR2_OUTPUT=# 3.706 3864603365258790656 162.50395651516 +06.53943997640 14.1937 13.1371 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52698_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 52698_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
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Considering the candidate 52717_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52717_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:38:08.09 +10:40:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 1.160 3916014806691355648 174.53341241083 +10.66688901791 14.4665 13.6022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52732_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52732_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:51:58.99 +07:09:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 2.286 3865402504053779072 162.99632714710 +07.16640316327 14.7392 14.1931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52734_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52734_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:47:50.63 +10:02:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 0.603 3869618100354141056 161.96112825323 +10.04870401837 14.5716 13.7208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52735_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52735_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:58:46.02 +07:16:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 1.974 3864888448008237824 164.69119755227 +07.26957774902 14.7861 14.3294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52739_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52739_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:25:36.04 +10:22:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 1.323 3915440110002820736 171.40052249147 +10.37108206151 14.9201 14.4588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52748_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 52748_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
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Considering the candidate 52751_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 52751_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
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Considering the candidate 52753_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52753_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:50:25.82 +08:06:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.508 3866074236939019520 162.60717588659 +08.10508538018 14.0375 12.8667 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52755_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52755_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:30:32.56 +10:23:39.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)
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Considering the candidate 52756_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52756_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:22:43.15 +01:59:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.58, MAG_FAINT_SEARCH_LIMIT=15.56)GAIADR2_OUTPUT=# 4.551 3810767049715469056 170.67890653831 +01.99320799952 14.2008 13.1176 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52761_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52761_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:12:01.47 +08:11:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 3.303 3818799016515952896 168.00520603963 +08.19082414934 14.7673 14.1005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52763_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52763_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:31:04.27 +10:55:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.902 3915510238228380672 172.76769730052 +10.92157271461 14.8907 13.9958 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.902#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52766_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52766_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:35:58.57 +01:08:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 0.557 3799111092589805184 173.99392055107 +01.13982041901 14.8021 14.3206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52769_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52769_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:40:26.54 +03:35:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 0.049 3857663728900783488 160.11059638199 +03.59289320316 14.6367 14.0016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52774_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 52774_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
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Considering the candidate 52778_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 52778_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
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Considering the candidate 52793_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52793_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:30:01.70 +08:36:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 3.449 3913883854373128320 172.50617654700 +08.60900430570 15.0888 14.5379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52796_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 52796_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
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Considering the candidate 52809_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
Preparing report for the candidate 52809_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
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Considering the candidate 52810_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52810_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:45:48.71 +06:48:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 2.219 3865315505196813952 161.45312920628 +06.80262030686 14.7991 14.2384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.219#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52813_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52813_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:39:45.44 +05:25:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52816_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52816_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:40:15.06 +10:08:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 0.851 3870364531310997888 160.06251300617 +10.14057272394 14.8629 14.2932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52823_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52823_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:31:29.97 +06:03:58.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)
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Considering the candidate 52828_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52828_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:46:03.98 +03:51:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 1.810 3857915654502406784 161.51610232100 +03.85031683034 14.8292 13.9788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52832_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52832_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:46:39.93 +07:39:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.654 3865668414069468800 161.66632679183 +07.65063036388 14.8597 14.3373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52834_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52834_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:00:36.47 +01:42:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 1.137 3805398718552396288 165.15169477014 +01.70528515860 14.7612 14.1020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52835_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52835_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:39:41.98 +07:55:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 0.974 3868693892111515264 159.92473523851 +07.92499223181 14.5985 14.1049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52837_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52837_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:54:13.89 +05:49:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.851 3864303061145653504 163.55780426926 +05.83178713417 15.0515 14.3237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52841_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52841_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:02:37.87 +01:03:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 0.414 3805299315829363968 165.65767727486 +01.06234449272 14.8190 14.3526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52843_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52843_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:39:07.56 +03:08:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 0.681 3800540457705936000 174.78131669921 +03.14925722413 14.7871 14.1724 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52848_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52848_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:09:22.41 +04:06:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 1.376 3815146473248313472 167.34346516061 +04.10985074436 15.1057 14.5696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52849_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52849_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:09:01.81 +06:20:01.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)
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Considering the candidate 52853_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52853_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:41:11.77 +08:50:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.691 3869045804552113664 160.29857586741 +08.83482319529 14.8684 14.3245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52856_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52856_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:49:57.49 +06:24:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 0.901 3864505336925385344 162.48953663953 +06.41349984607 14.7374 14.2068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52858_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52858_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 11:19:29.50 +01:37:12.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)
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Considering the candidate 52859_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52859_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:42:48.89 +03:36:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.555 3857558961763408768 160.70381291477 +03.60541908368 14.6613 14.1929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52867_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52867_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:51:01.89 +08:28:24.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)
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Considering the candidate 52879_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52879_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:41:59.64 +06:18:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 1.454 3859459742489388544 160.49842118302 +06.31307589879 14.7493 14.2274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52901_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52901_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:52:17.09 +05:01:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.704 3864096662197113728 163.07122077379 +05.02966568654 15.4158 14.9338 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52905_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52905_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:47:48.96 +01:50:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.238 3808979346887507328 161.95366652340 +01.84430385721 14.6003 14.0633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52926_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52926_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:37:43.05 +03:07:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.413 3856119189941426176 159.42911207552 +03.12631935086 14.8426 14.2995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52932_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52932_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
**** FOUND 10:42:52.42 +00:54:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 1.609 3807394572674804608 160.71802316408 +00.90189905879 14.5741 13.9370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52933_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158
The candidate 52933_fd_Leo-07-Q1b1x1_2026-03-22_02-13-16_20.00sec_-14.90C_LIGHT_0158 did not pass the final checks
