This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 11.2041* 05 18 05.76 +05 20 10.1 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0518060+052014,2461082.7041,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0518060+052014 20260211.2041 13.81CV 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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:05.76 +05:20:10.1 ;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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20_00sec_-15_00C_LIGHT_0163_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20_00sec_-15_00C_LIGHT_0162_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20_00sec_-15_00C_LIGHT_0163_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20_00sec_-15_00C_LIGHT_0162_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 02 11.2041* 05 38 26.45 +04 59 55.7 13.4 U Ori 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,2461082.7041,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260211.2041 13.38CV 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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:38:26.45 +04:59:55.7 ;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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20_00sec_-15_00C_LIGHT_0163_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20_00sec_-15_00C_LIGHT_0162_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20_00sec_-15_00C_LIGHT_0163_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20_00sec_-15_00C_LIGHT_0162_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 02 11.2041* 05 23 23.02 +08 39 55.0 13.5 U Ori 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,2461082.7041,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260211.2041 13.54CV 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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:23:23.02 +08:39:55.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20_00sec_-15_00C_LIGHT_0163_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20_00sec_-15_00C_LIGHT_0162_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20_00sec_-15_00C_LIGHT_0163_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20_00sec_-15_00C_LIGHT_0162_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 02 11.2041* 04 55 15.27 +08 14 01.7 14.2 U Ori 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,2461082.7041,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260211.2041 14.24CV 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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:55:15.27 +08:14:01.7 ;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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20_00sec_-15_00C_LIGHT_0163_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20_00sec_-15_00C_LIGHT_0162_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20_00sec_-15_00C_LIGHT_0163_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20_00sec_-15_00C_LIGHT_0162_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 02 11.2041* 05 15 02.71 +10 44 33.2 14.3 U Ori 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,2461082.7041,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260211.2041 14.35CV 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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:02.71 +10:44:33.2 ;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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20_00sec_-15_00C_LIGHT_0163_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20_00sec_-15_00C_LIGHT_0162_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20_00sec_-15_00C_LIGHT_0163_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20_00sec_-15_00C_LIGHT_0162_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 02 11.2041* 04 56 31.50 +05 35 33.7 13.9 U Ori 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
GO Ori,2461082.7041,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GO Ori 20260211.2041 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:31.50 +05:35:33.7 ;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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20_00sec_-15_00C_LIGHT_0163_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20_00sec_-15_00C_LIGHT_0162_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20_00sec_-15_00C_LIGHT_0163_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20_00sec_-15_00C_LIGHT_0162_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: 2461032.77884545 23.12.2025 06:41:22.247 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
First image: 2461032.77884545 23.12.2025 06:41:22.247 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
Last image: 2461082.70448678 11.02.2026 04:54:17.658 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
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: 4 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): 16388
Objects passed selection criteria: 16383
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 15826.2
Average stars matched: 15512 (98.0144 %)
Memory usage VmPeak: 123748 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Tue Feb 10 15:05:05 CST 2026
VaST build number 1.0rc88-299-g877bacc0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Feb 10 23:15:38 CST 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: 2461032.77884545 23.12.2025 06:41:22.247 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
First image: 2461032.77884545 23.12.2025 06:41:22.247 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
Last image: 2461082.70448678 11.02.2026 04:54:17.658 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 198
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
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: 51 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): 103926
Objects passed selection criteria: 103677
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: 99408.8
Average stars matched: 96314.2 (96.8871 %)
Memory usage VmPeak: 1888404 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Tue Feb 10 15:05:05 CST 2026
VaST build number 1.0rc88-299-g877bacc0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Feb 10 23:17:31 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
SExtractor catalog cache: saved Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat to cache
SExtractor catalog cache: saved Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.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: 2461082.70378047
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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits exists and is non-empty
Saving wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits to local_wcs_cache/
'wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits' -> 'local_wcs_cache/wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits'
wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits exists and is non-empty
Saving wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits to local_wcs_cache/
'wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits' -> 'local_wcs_cache/wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits'
wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits exists and is non-empty
Saving wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits to local_wcs_cache/
'wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits' -> 'local_wcs_cache/wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits'
wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits exists and is non-empty
Saving wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits to local_wcs_cache/
'wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits' -> 'local_wcs_cache/wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.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 05:08:17.653 +06:01:42.67
Second-epoch image center 05:08:31.714 +05:59:21.94
Angular distance between the image centers 0.07 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 05:08:17.653 +06:01:42.67
Second-epoch image center 05:08:29.022 +05:58:42.86
Angular distance between the image centers 0.07 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 05:08:31.714 +05:59:21.94
Second-epoch second image center 05:08:29.022 +05:58:42.86
Angular distance between the image centers 0.01557 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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits &> /tmp/tmp.M5vDf8ZjVb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits &> /tmp/tmp.G15xZO63Tk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits &> /tmp/tmp.N3yrGdqsC7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits &> /tmp/tmp.ecU4xRLmyD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits and wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits and wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
Found non-empty wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits and wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
The reference image (wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits) and catalog (wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat) found
'wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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 8346 out of 16639 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.941484
a=0.000000 b=1.000000 c=22.941484
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
____ 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:
2.0 pix Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
2.0 pix Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
2.3 pix fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
2.3 pix fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
Limiting magnitude estimates:
15.3 mag. Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
15.3 mag. Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
15.1 mag. fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
15.1 mag. fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.M5vDf8ZjVb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits' -> 'wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
WCS-calibrated image found: wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
Checking if the catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
WCS catalog name: wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1525, passed=16639
Got 16639 stars (including 15103 good ones) from the SExtractor catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
util/solve_plate_with_UCAC5 got 16639 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 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: 0.29"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits -region wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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.G15xZO63Tk (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits' -> 'wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
WCS-calibrated image found: wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
Checking if the catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
WCS catalog name: wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1536, passed=16598
Got 16598 stars (including 15044 good ones) from the SExtractor catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat
util/solve_plate_with_UCAC5 got 16598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits -region wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.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.N3yrGdqsC7 (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_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.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_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
Checking if the catalog wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
WCS catalog name: wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1364, passed=15192
Got 15192 stars (including 13813 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits.cat
util/solve_plate_with_UCAC5 got 15192 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 953 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits -region wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.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.ecU4xRLmyD (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_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.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_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
Checking if the catalog wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
WCS catalog name: wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1392, passed=15269
Got 15269 stars (including 13863 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits.cat
util/solve_plate_with_UCAC5 got 15269 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits -region wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.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_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits'
Saving fully-calibrated image wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits'
Preparing the HTML report for the field Ori-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20847.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
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 20847_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 20847_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:11:19.25 +09:20:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 1.404 3290608508300464000 077.83044395919 +09.34324257880 12.2505 11.6802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20924_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 20924_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:36:21.14 +09:29:27.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20945_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 20945_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:14:08.18 +05:57:44.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20958_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 20958_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:23:30.73 +03:47:30.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20961_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 20961_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:16:20.65 +07:42:20.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Ori-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
SExtractor catalog cache: saved Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat to cache
SExtractor catalog cache: saved Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
Creating symlink local_wcs_cache/wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits exists and is non-empty
wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits exists and is non-empty
wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits exists and is non-empty
wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.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 05:08:17.653 +06:01:42.67
Second-epoch image center 05:08:31.714 +05:59:21.94
Angular distance between the image centers 0.07 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 05:08:17.653 +06:01:42.67
Second-epoch image center 05:08:29.022 +05:58:42.86
Angular distance between the image centers 0.07 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 05:08:31.714 +05:59:21.94
Second-epoch second image center 05:08:29.022 +05:58:42.86
Angular distance between the image centers 0.01557 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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits &> /tmp/tmp.0TkwkXQOLJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits &> /tmp/tmp.87bV2MxpkM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits &> /tmp/tmp.g93xdnnwZR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits &> /tmp/tmp.F14aJmI3gg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits and wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits and wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
Found non-empty wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits and wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
The reference image (wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits) and catalog (wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat) found
'wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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 8481 out of 106531 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.798883
a=0.000000 b=1.000000 c=22.798883
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 50 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
1.9 pix Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
2.1 pix fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
2.2 pix fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
Limiting magnitude estimates:
15.5 mag. Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
15.5 mag. Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
15.2 mag. fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
15.2 mag. fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.0TkwkXQOLJ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits' -> 'wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
WCS-calibrated image found: wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
Checking if the catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
WCS catalog name: wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=9253, passed=106506
Got 106506 stars (including 97096 good ones) from the SExtractor catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
util/solve_plate_with_UCAC5 got 106506 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 955 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits -region wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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.87bV2MxpkM (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits' -> 'wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
WCS-calibrated image found: wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
Checking if the catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
WCS catalog name: wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=9240, passed=106589
Got 106589 stars (including 97168 good ones) from the SExtractor catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat
util/solve_plate_with_UCAC5 got 106589 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits -region wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.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.g93xdnnwZR (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_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.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_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
Checking if the catalog wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
WCS catalog name: wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=8496, passed=93876
Got 93876 stars (including 85238 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits.cat
util/solve_plate_with_UCAC5 got 93876 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits -region wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.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.F14aJmI3gg (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_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.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_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
Checking if the catalog wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
WCS catalog name: wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=8544, passed=93397
Got 93397 stars (including 84704 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits.cat
util/solve_plate_with_UCAC5 got 93397 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 956 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits -region wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.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_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.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_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-53-16_20.00sec_-15.00C_LIGHT_0162.fits
Saving fully-calibrated image wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.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_2026-02-10_CI_Ori-03-Q1b1x1_231320_TTUQ1b1x1_10135_wsWwryc3/wcs_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163.fits
Preparing the HTML report for the field Ori-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out125180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out125228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58263.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125171_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125171_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:32:55.61 +10:52:41.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125180_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125180_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:37:49.02 +07:33:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 3.573 3334379688245597184 084.45326430148 +07.56126973160 14.8122 14.2674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125201_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125201_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:34:46.81 +04:19:49.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125205_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125205_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:38:17.69 +01:41:14.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125207_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125207_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:06:09.50 +03:02:23.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125208_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125208_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 04:55:16.60 +10:37:06.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125210_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125210_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:33:18.51 +02:28:42.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125213_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125213_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:21:17.47 +00:54:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 0.606 3221742860941097600 080.32278617497 +00.90885964688 13.9719 13.4668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125215_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125215_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:24:41.81 +07:23:37.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125216_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125216_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:04:10.04 +01:19:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 1.846 3228942845333523200 076.04132049758 +01.32259265803 14.1114 13.6173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125219_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125219_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:02:51.25 +02:31:54.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125222_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125222_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:38:31.18 +03:52:20.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125224_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125224_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:39:10.28 +01:38:02.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125227_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125227_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 04:51:58.57 +07:15:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.732 3288945909280325376 072.99359504033 +07.25692331945 13.6964 12.8565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125228_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
Preparing report for the candidate 125228_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125236_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125236_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:31:49.42 +02:18:59.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125238_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125238_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:31:44.25 +05:47:57.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125239_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125239_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 04:44:01.07 +08:31:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.592 3292379752813209472 071.00444218925 +08.52430843511 13.1753 12.2619 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125241_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125241_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:35:41.77 +07:04:50.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125242_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125242_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:18:10.83 +03:59:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.099 3235548466377681024 079.54481902703 +03.99499243871 12.8944 12.3562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.099#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125243_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125243_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:22:04.69 +02:19:07.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125244_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125244_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 04:42:00.56 +08:04:01.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125245_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125245_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:09:26.46 +03:24:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 1.701 3235266686461008128 077.35983520378 +03.41628340542 12.8839 12.3975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125248_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125248_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:30:38.32 +01:49:03.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125348_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125348_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:33:39.39 +01:42:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.189 3223496861161809664 083.41409894217 +01.71598204417 12.2622 11.7305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125389_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125389_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:17:00.15 +02:44:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 0.826 3234559082008111744 079.25041303177 +02.73808844111 12.9301 12.4001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125471_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125471_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:20:57.66 +09:44:40.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125472_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125472_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:29:39.71 +01:56:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 0.794 3223735798781747456 082.41536641697 +01.93621612963 13.2313 12.7717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125484_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
Preparing report for the candidate 125484_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125485_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125485_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:29:11.13 +01:09:32.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125510_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
Preparing report for the candidate 125510_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125524_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125524_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 04:55:40.89 +02:21:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.118 3232234748787095168 073.92021185693 +02.36374033515 13.6665 13.0656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125547_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125547_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:17:08.26 +04:13:54.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125564_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125564_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:21:58.79 +03:28:55.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125615_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125615_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 04:42:45.37 +03:41:19.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125630_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125630_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 04:52:20.40 +01:12:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.032 3231661387833127936 073.08452920633 +01.21046640389 14.1443 13.5221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.032#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125681_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125681_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 04:46:24.43 +04:16:10.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125729_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
Preparing report for the candidate 125729_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125734_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
Preparing report for the candidate 125734_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125743_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125743_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:29:21.75 +06:32:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 2.318 3333882292375401984 082.34008973653 +06.54233130711 14.5390 13.7314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125756_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125756_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 04:38:12.04 +07:12:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 2.270 3286162010261577856 069.55077009583 +07.20369838320 14.7829 14.2532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125788_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125788_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:14:27.45 +00:58:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 2.229 3233715138114629120 078.61377386445 +00.97004584788 14.5091 13.9885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125802_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125802_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 04:39:59.02 +01:56:09.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125804_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125804_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:36:59.25 +01:59:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 2.007 3222871445202810752 084.24643489709 +01.98707394638 14.7213 14.0013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125808_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125808_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:33:48.99 +01:50:17.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125812_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125812_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 04:59:56.68 +02:36:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 1.238 3232160944069132928 074.98584370999 +02.60377018413 14.4594 13.8044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125814_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125814_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 04:55:33.92 +03:03:59.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125837_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 125837_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks
**** FOUND 05:24:25.95 +03:54:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.404 3236236283917095424 081.10812961187 +03.90819353858 14.6608 14.1685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16891_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163
The candidate 16891_fd_Ori-03-Q1b1x1_2026-02-10_22-54-17_20.00sec_-15.00C_LIGHT_0163 did not pass the final checks