This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2954* 12 50 46.53 -03 30 22.7 12.5 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7954,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2954 12.51CV 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/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:50:46.53 -03:30:22.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2954* 12 46 12.97 -06 06 42.1 12.6 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7954,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2954 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:46:12.97 -06:06:42.1 ;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_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2954* 12 29 11.53 -03 52 22.0 12.9 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7954,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2954 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:29:11.53 -03:52:22.0 ;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_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2954* 12 32 04.96 -03 02 55.7 13.9 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7954,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2954 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:32:04.96 -03:02:55.7 ;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_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2954* 12 39 03.87 +00 33 07.9 13.9 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7954,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2954 13.90CV 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/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:39:03.87 -00:33:07.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2954* 13 03 22.42 -04 44 28.4 14.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7954,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2954 14.44CV 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/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:03:22.42 -04:44:28.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2954* 12 40 13.07 -05 47 59.4 14.5 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7954,14.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2954 14.47CV 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/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:40:13.07 -05:47:59.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2954 2461121.7954 14.53 12:42:32.71 -01:21:00.4
298.27882 61.44127 galactic Vir Second-epoch detections are separated by 0.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:42:32.71 -01:21:00.4 (user input) | T | P | (position from user input) J-Ks=1.710+/- (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2954* 12 42 32.71 -01 21 00.4 14.5 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7954,14.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2954 14.53CV 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/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:42:32.71 -01:21:00.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2954* 12 24 24.26 +00 37 02.2 14.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7954,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2954 14.40CV 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/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:24:24.26 -00:37:02.2 ;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_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2954* 12 25 15.60 -01 52 04.8 14.6 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7954,14.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2954 14.59CV 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/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:25:15.60 -01:52:04.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20_00sec_-15_00C_LIGHT_0187_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20_00sec_-14_90C_LIGHT_0457_fits__*pix.png resample_wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20_00sec_-14_90C_LIGHT_0186_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.90824554 11.02.2026 09:47:42.415 /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
First image: 2461082.90824554 11.02.2026 09:47:42.415 /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
Last image: 2461121.79572319 22.03.2026 07:05:40.484 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.80
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5007
Objects passed selection criteria: 4999
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 4618.25
Average stars matched: 4243.75 (91.8909 %)
Memory usage VmPeak: 111448 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 02:46:19 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.90824554 11.02.2026 09:47:42.415 /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
First image: 2461082.90824554 11.02.2026 09:47:42.415 /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
Last image: 2461121.79572319 22.03.2026 07:05:40.484 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 68
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 14 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): 27883
Objects passed selection criteria: 27815
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: 27094.5
Average stars matched: 25456.8 (93.9554 %)
Memory usage VmPeak: 131596 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 02:47:09 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
SExtractor catalog cache: saved Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat to cache
SExtractor catalog cache: saved Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.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/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461121.79513062
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_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits exists and is non-empty
Saving wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits to local_wcs_cache/
'wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits' -> 'local_wcs_cache/wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits'
wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits exists and is non-empty
Saving wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits to local_wcs_cache/
'wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits' -> 'local_wcs_cache/wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits'
wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits exists and is non-empty
Saving wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits to local_wcs_cache/
'wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits' -> 'local_wcs_cache/wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits'
wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits exists and is non-empty
Saving wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits to local_wcs_cache/
'wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits' -> 'local_wcs_cache/wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.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 12:51:29.449 -01:59:42.64
Second-epoch image center 12:51:20.932 -01:59:25.19
Angular distance between the image centers 0.04 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 12:51:29.449 -01:59:42.64
Second-epoch image center 12:51:18.309 -01:59:24.48
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 12:51:20.932 -01:59:25.19
Second-epoch second image center 12:51:18.309 -01:59:24.48
Angular distance between the image centers 0.01092 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/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits &> /tmp/tmp.hDNGeSUoal
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits &> /tmp/tmp.JnWJnjawHz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits &> /tmp/tmp.Jvh5ZoNaeN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits &> /tmp/tmp.NNlriNKzmS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.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_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits and wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.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_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits and wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat
Found non-empty wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits and wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat
The reference image (wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits) and catalog (wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat) found
'wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.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 3192 out of 4824 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.791481
a=0.000000 b=1.000000 c=22.791481
From vast_summary.log: estimated ref. image limiting mag.: -7.80
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.99
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.99
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
2.1 pix Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
2.5 pix fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
2.4 pix fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
Limiting magnitude estimates:
15.0 mag. Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
15.0 mag. Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
15.1 mag. fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
15.2 mag. fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.hDNGeSUoal (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits' -> 'wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
WCS_IMAGE_NAME=wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
WCS-calibrated image found: wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
Checking if the catalog wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat corresponding to the image wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits alredy exist and is non-empty...
Catalog wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat corresponding to the image wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
WCS catalog name: wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=371, passed=4824
Got 4824 stars (including 4449 good ones) from the SExtractor catalog wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat
util/solve_plate_with_UCAC5 got 4824 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 984 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: 0.37"
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 984 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 984 stars left (next iteration limit 1082)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits -region wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.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.JnWJnjawHz (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits' -> 'wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
WCS_IMAGE_NAME=wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
WCS-calibrated image found: wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
Checking if the catalog wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat corresponding to the image wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits alredy exist and is non-empty...
Catalog wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat corresponding to the image wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
WCS catalog name: wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=372, passed=4941
Got 4941 stars (including 4564 good ones) from the SExtractor catalog wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat
util/solve_plate_with_UCAC5 got 4941 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 984 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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 984 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 984 stars left (next iteration limit 1082)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits -region wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.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.Jvh5ZoNaeN (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
WCS_IMAGE_NAME=wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
WCS-calibrated image found: wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
Checking if the catalog wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
WCS catalog name: wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=364, passed=6344
Got 6344 stars (including 5974 good ones) from the SExtractor catalog wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits.cat
util/solve_plate_with_UCAC5 got 6344 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 986 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 986 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: 0.34"
Excluding outliers - 986 stars left (next iteration limit 1084)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits -region wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.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.NNlriNKzmS (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
WCS_IMAGE_NAME=wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
WCS-calibrated image found: wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
Checking if the catalog wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits.cat corresponding to the image wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits.cat corresponding to the image wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
WCS catalog name: wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=370, passed=6259
Got 6259 stars (including 5885 good ones) from the SExtractor catalog wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits.cat
util/solve_plate_with_UCAC5 got 6259 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 986 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 986 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: 0.34"
Excluding outliers - 986 stars left (next iteration limit 1084)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits -region wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.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_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits'
Saving fully-calibrated image wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits'
Saving fully-calibrated image wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits'
Saving fully-calibrated image wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits'
Preparing the HTML report for the field Vir-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20303_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 20303_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 12:27:49.68 -03:59:08.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20304_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 20304_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 12:55:32.16 +00:03:42.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20307_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 20307_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 12:50:26.54 -02:25:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20308_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 20308_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 12:58:48.52 -01:54:05.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Vir-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
SExtractor catalog cache: saved Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat to cache
SExtractor catalog cache: saved Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
Creating symlink local_wcs_cache/wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.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_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits exists and is non-empty
wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits exists and is non-empty
wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits exists and is non-empty
wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.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 12:51:29.449 -01:59:42.64
Second-epoch image center 12:51:20.932 -01:59:25.19
Angular distance between the image centers 0.04 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 12:51:29.449 -01:59:42.64
Second-epoch image center 12:51:18.309 -01:59:24.48
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 12:51:20.932 -01:59:25.19
Second-epoch second image center 12:51:18.309 -01:59:24.48
Angular distance between the image centers 0.01092 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/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits &> /tmp/tmp.zht2Yu93bl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits &> /tmp/tmp.4nTQSCzVmG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits &> /tmp/tmp.ehM6oQQ33R
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits &> /tmp/tmp.C1m8WTxmay
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.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_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits and wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.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_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits and wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat
Found non-empty wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits and wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat
The reference image (wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits) and catalog (wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat) found
'wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.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 3394 out of 30136 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.653721
a=0.000000 b=1.000000 c=22.653721
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.16
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.16
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 49 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
1.9 pix Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
2.4 pix fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
2.3 pix fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
Limiting magnitude estimates:
15.2 mag. Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
15.2 mag. Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
15.3 mag. fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
15.3 mag. fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.zht2Yu93bl (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits' -> 'wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
WCS_IMAGE_NAME=wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
WCS-calibrated image found: wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
Checking if the catalog wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat corresponding to the image wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits alredy exist and is non-empty...
Catalog wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat corresponding to the image wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
WCS catalog name: wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1111, passed=30122
Got 30122 stars (including 28960 good ones) from the SExtractor catalog wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat
util/solve_plate_with_UCAC5 got 30122 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 983 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: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 983 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 983 stars left (next iteration limit 1081)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits -region wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.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.4nTQSCzVmG (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits' -> 'wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
WCS_IMAGE_NAME=wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
WCS-calibrated image found: wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
Checking if the catalog wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat corresponding to the image wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits alredy exist and is non-empty...
Catalog wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat corresponding to the image wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
WCS catalog name: wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1189, passed=30759
Got 30759 stars (including 29532 good ones) from the SExtractor catalog wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat
util/solve_plate_with_UCAC5 got 30759 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 983 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: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 983 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 983 stars left (next iteration limit 1081)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits -region wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.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.ehM6oQQ33R (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
WCS_IMAGE_NAME=wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
WCS-calibrated image found: wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
Checking if the catalog wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
WCS catalog name: wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1325, passed=31899
Got 31899 stars (including 30527 good ones) from the SExtractor catalog wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits.cat
util/solve_plate_with_UCAC5 got 31899 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 986 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 986 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 - 986 stars left (next iteration limit 1084)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits -region wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.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.C1m8WTxmay (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
WCS_IMAGE_NAME=wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
WCS-calibrated image found: wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
Checking if the catalog wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits.cat corresponding to the image wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits.cat corresponding to the image wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
WCS catalog name: wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1342, passed=32601
Got 32601 stars (including 31217 good ones) from the SExtractor catalog wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits.cat
util/solve_plate_with_UCAC5 got 32601 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 986 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: 0.37"
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 986 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 986 stars left (next iteration limit 1084)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits -region wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.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_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/wcs_Vir-07-Q2b1x1_2026-02-11_03-47-42_20.00sec_-14.90C_LIGHT_0457.fits
Saving fully-calibrated image wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/wcs_Vir-07-Q2b1x1_2026-02-11_03-48-36_20.00sec_-15.00C_LIGHT_0458.fits
Saving fully-calibrated image wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-04-49_20.00sec_-14.90C_LIGHT_0186.fits
Saving fully-calibrated image wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Vir-07-Q2b1x1_024120_TTUQ2b1x1_2986_dKJzxYZ5/wcs_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187.fits
Preparing the HTML report for the field Vir-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52655.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52714.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out52681.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out52331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52847.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
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: 7s
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Considering the candidate 52296_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52296_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 12:57:18.35 -01:22:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)GAIADR2_OUTPUT=# 1.366 3688664015708202496 194.32683004522 -01.36771509645 14.5145 13.9104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52297_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52297_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:08:17.23 +01:29:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 2.114 3691134480896977664 197.07233698224 +01.48794056008 14.4501 13.7026 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52298_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52298_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 52331_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
Preparing report for the candidate 52331_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
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Considering the candidate 52336_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
Preparing report for the candidate 52336_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
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Considering the candidate 52375_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
Preparing report for the candidate 52375_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
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Considering the candidate 52536_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
Preparing report for the candidate 52536_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
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Considering the candidate 52542_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
Preparing report for the candidate 52542_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
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Considering the candidate 52582_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52582_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:13:58.74 -02:45:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52598_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52598_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 52622_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52622_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:15:34.51 +00:29:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 0.890 3687601234640609920 198.89377363400 +00.48455895358 14.5072 14.0201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52629_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52629_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:06:22.15 -01:40:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52631_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52631_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:15:29.17 +00:12:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)GAIADR2_OUTPUT=# 1.674 3687574915081011456 198.87199496157 +00.20100681561 14.5068 13.6896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52642_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52642_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:11:11.38 -02:09:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52646_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52646_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:01:46.23 -06:17:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 1.064 3629323648035005440 195.44290342294 -06.28915967990 14.7512 14.2091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52650_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52650_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:11:37.41 -03:52:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 3.185 3684097022363474176 197.90610096290 -03.87802210989 14.9179 14.4654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52652_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
Preparing report for the candidate 52652_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
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Considering the candidate 52653_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52653_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:14:14.48 +02:06:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52655_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52655_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:06:30.80 -05:50:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 0.998 3629684425287907200 196.62855676334 -05.83411223478 14.5293 14.0238 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52670_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52670_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:09:05.68 +02:13:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 1.205 3691618094214246912 197.27375830304 +02.22795576454 14.6186 14.0966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52674_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52674_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:11:59.18 +00:49:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 0.902 3687848556037305728 197.99682360943 +00.82582100082 14.6500 14.0848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.902#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52678_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52678_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 12:56:59.71 -05:57:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52680_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52680_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:13:16.69 +00:09:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 1.491 3687748122522116608 198.31995113742 +00.15513278448 14.7218 14.0060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52681_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52681_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:13:52.33 +02:07:56.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)
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Considering the candidate 52682_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
Preparing report for the candidate 52682_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
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Considering the candidate 52683_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52683_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:05:59.64 -06:13:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 1.955 3629656250302427264 196.49896105130 -06.21923560497 14.6925 14.2094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52687_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52687_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:12:54.28 +01:16:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 1.051 3691264257628604288 198.22635945123 +01.26738612414 14.9162 14.2909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52693_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52693_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:15:21.48 +01:55:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52697_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52697_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:15:17.68 +01:24:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 1.081 3688290594071638272 198.82387233495 +01.40914227005 14.8318 14.3592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52700_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52700_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:15:08.09 -00:22:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)GAIADR2_OUTPUT=# 1.387 3687481765830278784 198.78409291703 -00.38088636036 14.7614 14.3612 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52702_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52702_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 12:33:06.43 -06:00:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52707_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
Preparing report for the candidate 52707_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
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Considering the candidate 52711_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52711_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:08:14.77 -01:23:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)GAIADR2_OUTPUT=# 0.591 3685755979251338752 197.06169271492 -01.38988031666 14.7436 14.2668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52714_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52714_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:14:45.32 +01:58:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 1.898 3691328613418645504 198.68935990543 +01.97804944264 14.6521 14.1251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52715_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52715_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:11:06.91 +00:51:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 0.974 3690851322292870656 197.77904251705 +00.86134318162 14.5229 14.0894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52716_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52716_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:04:21.50 -05:46:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 1.766 3629731871790727808 196.09007128390 -05.77740092783 14.4410 13.8080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52720_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52720_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:12:00.10 +01:44:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52737_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52737_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:06:35.04 -04:20:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 1.200 3684017926245824256 196.64633414754 -04.33823762677 14.7243 14.3228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52746_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52746_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 12:51:11.18 -04:39:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 0.793 3678552288303923968 192.79680039354 -04.66426379170 14.5469 14.0089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52753_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52753_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:02:27.32 -04:21:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 0.974 3678191648490113408 195.61358037643 -04.36612420546 14.9431 14.4464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52769_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52769_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 52778_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52778_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 12:36:00.44 -04:53:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 1.236 3680364661423844224 189.00212795884 -04.89409971851 14.7581 14.4012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52785_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52785_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 13:10:34.03 +01:48:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 0.568 3691356754044225408 197.64191103405 +01.81059138948 14.8000 14.2770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52798_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
Preparing report for the candidate 52798_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
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Considering the candidate 52801_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52801_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 12:24:42.52 -05:09:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.57, MAG_FAINT_SEARCH_LIMIT=15.55)GAIADR2_OUTPUT=# 1.259 3680866725921339392 186.17751167806 -05.15414869086 14.6251 14.0240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52847_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
Preparing report for the candidate 52847_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
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Considering the candidate 52861_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52861_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 12:23:52.25 -05:42:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 0.831 3584548579614895360 185.96754540773 -05.70480320978 14.7588 14.1513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52931_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52931_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks
**** FOUND 12:24:14.65 -04:18:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 2.914 3692990834483136384 186.06184076669 -04.31011375718 14.9667 14.3472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52945_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187
The candidate 52945_fd_Vir-07-Q2b1x1_2026-03-22_02-05-40_20.00sec_-15.00C_LIGHT_0187 did not pass the final checks