This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 19.3483 2461118.8483 13.76 09:15:34.82 +18:20:27.1
211.03445 39.82588 galactic Cnc Second-epoch detections are separated by 3.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:15:34.82 +18:20:27.1 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461118.8483,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3483 13.76CV 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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:15:34.82 +18:20:27.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3483* 09 55 55.80 +15 29 46.2 12.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8483,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3483 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:55:55.80 +15:29:46.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3483* 09 45 05.37 +17 05 00.6 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,2461118.8483,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3483 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:45:05.37 +17:05:00.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3483 2461118.8483 14.09 09:15:17.06 +18:32:41.7
210.75354 39.83103 galactic Cnc Second-epoch detections are separated by 3.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:15:17.06 +18:32:41.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461118.8483,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3483 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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:15:17.06 +18:32:41.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3483* 09 28 25.10 +12 23 57.7 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,2461118.8483,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3483 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:28:25.10 +12:23:57.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.3483* 09 46 33.02 +16 32 26.8 14.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8483,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.3483 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:46:33.02 +16:32:26.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20_00sec_-15_00C_LIGHT_0079_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20_00sec_-15_00C_LIGHT_0229_fits__*pix.png resample_wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.73802228 09.01.2026 05:42:35.125 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
First image: 2461049.73802228 09.01.2026 05:42:35.125 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Last image: 2461118.84859003 19.03.2026 08:21:48.179 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.75
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 7236
Objects passed selection criteria: 7231
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: 6779.75
Average stars matched: 6485.75 (95.6636 %)
Memory usage VmPeak: 116044 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 03:31:59 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: 2461049.73802228 09.01.2026 05:42:35.125 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
First image: 2461049.73802228 09.01.2026 05:42:35.125 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Last image: 2461118.84859003 19.03.2026 08:21:48.179 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 109
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 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): 38441
Objects passed selection criteria: 38356
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: 36652.2
Average stars matched: 35088.8 (95.7342 %)
Memory usage VmPeak: 138640 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 03:32:48 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
SExtractor catalog cache: saved Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461118.84803373
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits exists and is non-empty
Saving wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits to local_wcs_cache/
'wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits' -> 'local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits'
wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits exists and is non-empty
Saving wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits to local_wcs_cache/
'wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits' -> 'local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits'
wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits exists and is non-empty
Saving wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits to local_wcs_cache/
'wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits' -> 'local_wcs_cache/wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits'
wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits exists and is non-empty
Saving wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits to local_wcs_cache/
'wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits' -> 'local_wcs_cache/wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:46:15.747 +13:59:46.03
Second-epoch image center 09:46:55.083 +14:00:35.75
Angular distance between the image centers 0.16 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:46:15.747 +13:59:46.03
Second-epoch image center 09:46:53.044 +14:00:41.78
Angular distance between the image centers 0.15 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:46:55.083 +14:00:35.75
Second-epoch second image center 09:46:53.044 +14:00:41.78
Angular distance between the image centers 0.00841 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits &> /tmp/tmp.Yx9MOdcLQn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits &> /tmp/tmp.gPyRWalOK6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits &> /tmp/tmp.KxwxSNkJFG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits &> /tmp/tmp.FOvLPqeB9D
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits and wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits and wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
Found non-empty wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits and wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
The reference image (wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits) and catalog (wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat) found
'wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 4091 out of 6614 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.851467
a=0.000000 b=1.000000 c=22.851467
From vast_summary.log: estimated ref. image limiting mag.: -7.75
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.10
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.10
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
2.0 pix Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
2.5 pix fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
2.4 pix fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
Limiting magnitude estimates:
15.1 mag. Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
15.1 mag. Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
15.1 mag. fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
15.1 mag. fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Yx9MOdcLQn (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits' -> 'wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=440, passed=6614
Got 6614 stars (including 6163 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
util/solve_plate_with_UCAC5 got 6614 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.26"
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 911 stars left (next iteration limit 1002)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits -region wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.gPyRWalOK6 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits' -> 'wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=457, passed=6505
Got 6505 stars (including 6040 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat
util/solve_plate_with_UCAC5 got 6505 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 914 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits -region wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.KxwxSNkJFG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
Checking if the catalog wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
WCS catalog name: wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=378, passed=7126
Got 7126 stars (including 6744 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits.cat
util/solve_plate_with_UCAC5 got 7126 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 911 stars left (next iteration limit 1002)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits -region wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.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.FOvLPqeB9D (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
Checking if the catalog wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
WCS catalog name: wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=393, passed=7047
Got 7047 stars (including 6646 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits.cat
util/solve_plate_with_UCAC5 got 7047 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 912 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits -region wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits'
Saving fully-calibrated image wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits'
Saving fully-calibrated image wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits'
Saving fully-calibrated image wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits'
Preparing the HTML report for the field Leo-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20349.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20349_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 20349_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:16:35.29 +09:28:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 2.518 590672631582907520 139.14644872356 +09.47506080973 11.8582 11.1767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20363_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 20363_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:40:58.97 +09:52:40.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20369_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 20369_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:36:21.41 +13:37:21.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20370_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 20370_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:40:52.24 +14:14:04.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20372_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 20372_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:42:27.61 +13:47:18.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Leo-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
SExtractor catalog cache: saved Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Creating symlink local_wcs_cache/wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits exists and is non-empty
wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits exists and is non-empty
wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits exists and is non-empty
wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:46:15.747 +13:59:46.03
Second-epoch image center 09:46:55.083 +14:00:35.75
Angular distance between the image centers 0.16 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:46:15.747 +13:59:46.03
Second-epoch image center 09:46:53.044 +14:00:41.78
Angular distance between the image centers 0.15 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:46:55.083 +14:00:35.75
Second-epoch second image center 09:46:53.044 +14:00:41.78
Angular distance between the image centers 0.00841 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits &> /tmp/tmp.7qb33VKbZM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits &> /tmp/tmp.7S8HSlp2yc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits &> /tmp/tmp.nQbDtZDw26
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits &> /tmp/tmp.CoyIu8rMrk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits and wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits and wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
Found non-empty wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits and wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
The reference image (wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits) and catalog (wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat) found
'wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 4172 out of 37606 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.734542
a=0.000000 b=1.000000 c=22.734542
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.24
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.24
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 40 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
1.9 pix Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
2.3 pix fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
2.3 pix fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
Limiting magnitude estimates:
15.2 mag. Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
15.3 mag. Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
15.2 mag. fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
15.2 mag. fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.7qb33VKbZM (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits' -> 'wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1467, passed=37598
Got 37598 stars (including 36067 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat
util/solve_plate_with_UCAC5 got 37598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 909 stars left (next iteration limit 999)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits -region wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.7S8HSlp2yc (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits' -> 'wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WCS-calibrated image found: wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
Checking if the catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat corresponding to the image wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
WCS catalog name: wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1514, passed=38235
Got 38235 stars (including 36667 good ones) from the SExtractor catalog wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat
util/solve_plate_with_UCAC5 got 38235 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 909 stars left (next iteration limit 999)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits -region wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nQbDtZDw26 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
Checking if the catalog wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
WCS catalog name: wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1485, passed=35675
Got 35675 stars (including 34149 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits.cat
util/solve_plate_with_UCAC5 got 35675 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 910 stars left (next iteration limit 1001)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits -region wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.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.CoyIu8rMrk (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
Checking if the catalog wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits.cat corresponding to the image wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
WCS catalog name: wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1507, passed=36086
Got 36086 stars (including 34538 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits.cat
util/solve_plate_with_UCAC5 got 36086 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 912 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits -region wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.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-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/wcs_Leo-04-Q2b1x1_2026-01-08_23-42-35_20.00sec_-15.00C_LIGHT_0229.fits
Saving fully-calibrated image wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/wcs_Leo-04-Q2b1x1_2026-01-08_23-43-27_20.00sec_-14.90C_LIGHT_0230.fits
Saving fully-calibrated image wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-00_20.00sec_-14.90C_LIGHT_0078.fits
Saving fully-calibrated image wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Leo-04-Q2b1x1_032942_TTUQ2b1x1_8152_rF7A0OaY/wcs_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079.fits
Preparing the HTML report for the field Leo-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out50030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52988.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53003.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53016.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out53612.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out53008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53581.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
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
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Considering the candidate 52982_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 52982_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 10:15:51.07 +15:01:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 0.690 3888012998606311168 153.96262555758 +15.03183940316 14.5496 13.9957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52987_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 52987_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 10:00:04.08 +09:59:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 1.478 3878565444944438016 150.01662640821 +09.98337351706 14.0304 13.3438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52988_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 52988_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:15:20.84 +16:58:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 3.663 631967092866432000 138.83577197976 +16.96753971995 13.8583 13.3582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52992_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 52992_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 10:16:43.47 +12:30:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.684 3886694581085386240 154.18156088930 +12.50655585093 14.2087 13.5915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52993_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 52993_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:18:18.55 +18:53:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 4.799 635632486676356480 139.57863733296 +18.88746612272 13.7577 13.0891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52994_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 52994_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:26:20.49 +09:57:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 0.095 589245809087412736 141.58539624207 +09.95365476137 14.3104 13.8201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52996_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 52996_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:15:28.23 +12:56:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.092 605910071741886208 138.86793571123 +12.94346347535 13.6084 12.9645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52997_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 52997_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:19:52.38 +18:42:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 3.521 632610027995136256 139.96927958206 +18.71663193600 13.5692 12.9029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52998_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 52998_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:15:04.04 +17:16:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 3.328 632029146553831168 138.76780147641 +17.27033311692 13.7359 13.2376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53000_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53000_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:22:28.05 +13:41:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 0.701 594362936203120896 140.61707378580 +13.68844221690 13.9433 13.3837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53001_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53001_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:15:45.62 +17:11:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.911 631980287005954944 138.93961713089 +17.19954455432 13.5724 13.1382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53002_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53002_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 53003_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53003_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:16:05.39 +16:23:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 2.576 631716094978024192 139.02173083664 +16.39368626275 13.5700 12.9854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53006_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53006_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 10:09:01.91 +09:34:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.230 3876839585350726912 152.25804101686 +09.57277940163 13.7662 13.2816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53008_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 53008_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 53011_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53011_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:51:07.14 +16:14:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53012_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53012_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:15:20.59 +16:37:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 2.397 631735233352262912 138.83646187872 +16.61651869749 12.6072 11.9383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53015_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53015_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 10:16:44.39 +18:22:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 0.714 624097471533947520 154.18501096156 +18.37025255024 12.6760 11.9989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53016_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53016_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:43:26.13 +12:59:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 0.644 614496196698483712 145.85894496397 +12.99591546585 12.5333 12.0237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53119_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 53119_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 53183_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53183_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:39:00.86 +14:25:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53197_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 53197_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 53287_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53287_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:41:18.05 +09:36:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 0.530 588507968065410304 145.32509670934 +09.60315210719 13.4082 12.6240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53298_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53298_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:17:20.82 +16:32:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.406 631739425240361088 139.33605872774 +16.53533096807 13.3026 12.5724 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53444_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 53444_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 53453_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53453_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:30:14.24 +12:51:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53468_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53468_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:19:23.86 +10:09:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 3.191 591003103546242816 139.84882667634 +10.16588579453 13.9360 13.2019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53529_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 53529_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 53558_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53558_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 10:17:41.94 +10:59:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 0.610 3877383328210380800 154.42492082627 +10.98833020311 14.1489 13.5603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53576_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53576_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 10:17:49.15 +16:39:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.454 3888846011807827328 154.45468157371 +16.65438777077 14.2411 13.7867 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 53579_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53579_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:30:13.02 +12:51:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 0.221 617292735804069504 142.55422442915 +12.85872173071 14.3469 13.9099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53581_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
Preparing report for the candidate 53581_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
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Considering the candidate 53597_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53597_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:25:12.47 +14:47:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 4.621 618526662728555264 141.30236640305 +14.79569517351 14.4268 13.7950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53612_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53612_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 09:51:01.46 +11:52:31.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)
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Considering the candidate 53616_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53616_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 10:18:16.63 +15:00:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.495 3888375077234098432 154.56944343946 +15.00183365116 14.5047 13.9779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53722_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53722_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 10:16:20.25 +12:23:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.784 3880677160104736000 154.08487144190 +12.39937014097 14.5163 14.0149 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.784#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53734_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53734_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 10:03:58.78 +18:55:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 1.524 626615147003123840 150.99472694560 +18.91758893846 14.4900 13.9639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53745_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53745_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 10:12:40.18 +13:29:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 1.489 3887750765083165696 153.16723078817 +13.49273912160 14.5475 14.0327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53856_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 53856_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks
**** FOUND 10:14:50.84 +13:00:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 0.869 3886959047991881600 153.71158757808 +13.01341883964 14.3944 13.8328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 50030_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079
The candidate 50030_fd_Leo-04-Q2b1x1_2026-03-19_03-21-48_20.00sec_-15.00C_LIGHT_0079 did not pass the final checks