This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.3734* 14 30 11.30 -03 52 46.8 11.1 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.8734,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.3734 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:30:11.30 -03:52:46.8 ;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-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20_00sec_-15_00C_LIGHT_0429_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20_00sec_-15_00C_LIGHT_0428_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20_00sec_-15_00C_LIGHT_0428_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.3734 2461093.8734 12.84 14:42:41.36 -05:57:42.4
346.16730 47.35415 galactic Vir Second-epoch detections are separated by 7.6" and 8.2 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 | Gaia DR3 6331686593590409216 | 14:42:39.91 -05:57:51.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
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 02 22.3734* 14 42 41.36 -05 57 42.4 12.8 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
Gaia DR3 6331686593590409216,2461093.8734,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6331686593590409216 20260222.3734 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:42:41.36 -05:57:42.4 ;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-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20_00sec_-15_00C_LIGHT_0429_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20_00sec_-15_00C_LIGHT_0428_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20_00sec_-15_00C_LIGHT_0428_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.3734* 14 33 55.10 -03 08 06.4 13.8 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,2461093.8734,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.3734 13.79CV 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-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:33:55.10 -03:08:06.4 ;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-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20_00sec_-15_00C_LIGHT_0429_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20_00sec_-15_00C_LIGHT_0428_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20_00sec_-15_00C_LIGHT_0428_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.3734 2461093.8734 14.22 15:04:31.81 -04:36:29.2
353.38778 44.83352 galactic Lib Second-epoch detections are separated by 3.7" and 8.6 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 | 15:04:31.81 -04:36:29.2 (user input) | T | P | (position from user input) J-Ks=1.331+/-0.177 (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!
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,2461093.8734,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.3734 14.22CV 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-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:04:31.81 -04:36:29.2 ;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-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20_00sec_-15_00C_LIGHT_0429_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20_00sec_-15_00C_LIGHT_0428_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20_00sec_-15_00C_LIGHT_0428_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.3734* 14 45 29.02 -04 01 16.0 13.1 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CZ Vir,2461093.8734,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CZ Vir 20260222.3734 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:45:29.02 -04:01:16.0 ;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-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20_00sec_-15_00C_LIGHT_0429_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20_00sec_-15_00C_LIGHT_0428_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20_00sec_-15_00C_LIGHT_0429_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png resample_wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20_00sec_-15_00C_LIGHT_0428_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: 2461082.91090164 11.02.2026 09:51:31.902 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
First image: 2461082.91090164 11.02.2026 09:51:31.902 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
Last image: 2461093.87366517 22.02.2026 08:57:54.671 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.89
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5868
Objects passed selection criteria: 5865
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 5650.5
Average stars matched: 5358.75 (94.8367 %)
Memory usage VmPeak: 112016 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 03:04:21 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.91090164 11.02.2026 09:51:31.902 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
First image: 2461082.91090164 11.02.2026 09:51:31.902 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
Last image: 2461093.87366517 22.02.2026 08:57:54.671 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 151
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.59
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: 22 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): 37201
Objects passed selection criteria: 37117
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: 35962.2
Average stars matched: 34254.8 (95.252 %)
Memory usage VmPeak: 138008 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 03:05:54 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
SExtractor catalog cache: saved Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat to cache
SExtractor catalog cache: saved Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.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-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.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: 2461093.87318156
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-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits exists and is non-empty
Saving wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits to local_wcs_cache/
'wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits' -> 'local_wcs_cache/wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits'
wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits exists and is non-empty
Saving wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits to local_wcs_cache/
'wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits' -> 'local_wcs_cache/wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits'
wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits exists and is non-empty
Saving wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits to local_wcs_cache/
'wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits' -> 'local_wcs_cache/wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits'
wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits exists and is non-empty
Saving wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits to local_wcs_cache/
'wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits' -> 'local_wcs_cache/wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.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 14:34:17.527 -02:00:11.21
Second-epoch image center 14:34:17.731 -01:59:55.45
Angular distance between the image centers 0.00 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 14:34:17.527 -02:00:11.21
Second-epoch image center 14:34:20.473 -02:00:26.58
Angular distance between the image centers 0.01 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 14:34:17.731 -01:59:55.45
Second-epoch second image center 14:34:20.473 -02:00:26.58
Angular distance between the image centers 0.01432 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-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits &> /tmp/tmp.mvOyoIKBTD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits &> /tmp/tmp.5OdiodOLMf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits &> /tmp/tmp.cTkLBN5riW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits &> /tmp/tmp.dTHKaiHw4r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.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-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits and wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.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-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits and wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat
Found non-empty wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits and wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat
The reference image (wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits) and catalog (wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat) found
'wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.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 3336 out of 5265 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.784295
a=0.000000 b=1.000000 c=22.784295
From vast_summary.log: estimated ref. image limiting mag.: -7.89
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.89
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
2.1 pix Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
2.3 pix fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
2.3 pix fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
Limiting magnitude estimates:
14.9 mag. Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
14.9 mag. Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
15.0 mag. fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
15.0 mag. fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.mvOyoIKBTD (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.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-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits' -> 'wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
WCS_IMAGE_NAME=wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
WCS-calibrated image found: wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
Checking if the catalog wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits alredy exist and is non-empty...
Catalog wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
WCS catalog name: wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=424, passed=5265
Got 5265 stars (including 4833 good ones) from the SExtractor catalog wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat
util/solve_plate_with_UCAC5 got 5265 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 932 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: 0.35"
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 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits -region wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.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.5OdiodOLMf (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.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-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits' -> 'wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
WCS_IMAGE_NAME=wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
WCS-calibrated image found: wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
Checking if the catalog wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits alredy exist and is non-empty...
Catalog wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
WCS catalog name: wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=418, passed=5379
Got 5379 stars (including 4952 good ones) from the SExtractor catalog wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits.cat
util/solve_plate_with_UCAC5 got 5379 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 932 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: 0.36"
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 932 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: 0.34"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits -region wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.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.cTkLBN5riW (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
WCS_IMAGE_NAME=wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
WCS-calibrated image found: wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
Checking if the catalog wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
WCS catalog name: wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=434, passed=6056
Got 6056 stars (including 5613 good ones) from the SExtractor catalog wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits.cat
util/solve_plate_with_UCAC5 got 6056 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 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: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits -region wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.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.dTHKaiHw4r (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
WCS_IMAGE_NAME=wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
WCS-calibrated image found: wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
Checking if the catalog wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
WCS catalog name: wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=435, passed=6073
Got 6073 stars (including 5629 good ones) from the SExtractor catalog wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat
util/solve_plate_with_UCAC5 got 6073 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 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: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits -region wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits'
Saving fully-calibrated image wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits'
Preparing the HTML report for the field Vir-09-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20380.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20380_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
Preparing report for the candidate 20380_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20384_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 20384_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:36:21.74 -04:09:52.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Vir-09-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
14:30:11.30 -03:52:46.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
SExtractor catalog cache: saved Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat to cache
SExtractor catalog cache: saved Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.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-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
Creating symlink local_wcs_cache/wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.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-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits exists and is non-empty
wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits exists and is non-empty
wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits exists and is non-empty
wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.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 14:34:17.527 -02:00:11.21
Second-epoch image center 14:34:17.731 -01:59:55.45
Angular distance between the image centers 0.00 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 14:34:17.527 -02:00:11.21
Second-epoch image center 14:34:20.473 -02:00:26.58
Angular distance between the image centers 0.01 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 14:34:17.731 -01:59:55.45
Second-epoch second image center 14:34:20.473 -02:00:26.58
Angular distance between the image centers 0.01432 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-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits &> /tmp/tmp.AgbcIxdzvC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits &> /tmp/tmp.BAxNIQn3Oq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits &> /tmp/tmp.mz7BL8VqFH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits &> /tmp/tmp.16wpBWG3S5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.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-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits and wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.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-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits and wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat
Found non-empty wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits and wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat
The reference image (wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits) and catalog (wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat) found
'wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.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 3567 out of 35230 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.630463
a=0.000000 b=1.000000 c=22.630463
From vast_summary.log: estimated ref. image limiting mag.: -7.59
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 52 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
2.0 pix Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
2.2 pix fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
2.2 pix fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
Limiting magnitude estimates:
15.0 mag. Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
15.1 mag. Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
15.1 mag. fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
15.1 mag. fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.AgbcIxdzvC (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.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-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits' -> 'wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
WCS_IMAGE_NAME=wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
WCS-calibrated image found: wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
Checking if the catalog wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits alredy exist and is non-empty...
Catalog wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits
WCS catalog name: wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1362, passed=35217
Got 35217 stars (including 33783 good ones) from the SExtractor catalog wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat
util/solve_plate_with_UCAC5 got 35217 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 928 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 928 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 - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits -region wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-09-Q1b1x1_2026-02-11_03-51-31_20.00sec_-14.90C_LIGHT_0461.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.BAxNIQn3Oq (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.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-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits' -> 'wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
WCS_IMAGE_NAME=wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
WCS-calibrated image found: wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
Checking if the catalog wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits alredy exist and is non-empty...
Catalog wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits.cat corresponding to the image wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits
WCS catalog name: wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1361, passed=35580
Got 35580 stars (including 34152 good ones) from the SExtractor catalog wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits.cat
util/solve_plate_with_UCAC5 got 35580 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 927 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: 0.37"
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 927 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 - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits -region wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-09-Q1b1x1_2026-02-11_03-52-10_20.00sec_-14.90C_LIGHT_0462.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.mz7BL8VqFH (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
WCS_IMAGE_NAME=wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
WCS-calibrated image found: wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
Checking if the catalog wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
WCS catalog name: wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1642, passed=37173
Got 37173 stars (including 35460 good ones) from the SExtractor catalog wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits.cat
util/solve_plate_with_UCAC5 got 37173 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 928 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 928 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: 0.33"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits -region wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.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.16wpBWG3S5 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
WCS_IMAGE_NAME=wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
WCS-calibrated image found: wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
Checking if the catalog wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat corresponding to the image wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
WCS catalog name: wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1644, passed=37113
Got 37113 stars (including 35400 good ones) from the SExtractor catalog wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat
util/solve_plate_with_UCAC5 got 37113 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 928 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 928 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: 0.33"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits -region wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-12_20.00sec_-15.00C_LIGHT_0428.fits
Saving fully-calibrated image wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-09-Q1b1x1_025841_TTUQ1b1x1_11467_cgG9SSfV/wcs_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429.fits
Preparing the HTML report for the field Vir-09-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53136.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53141.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53145.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53147.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53176.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53177.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53184.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53219.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53291.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out53241.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out10979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53128.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 23s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 53086_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53086_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:13:15.38 +00:16:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 0.900 3659995349525460480 213.31425372275 +00.27296064664 14.5970 13.9467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53087_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53087_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:12:25.91 +02:54:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 1.808 3667336067109622144 213.10777290914 +02.91507789414 14.4091 14.1228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53088_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53088_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:57:18.43 +01:54:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 2.394 1154189967363853824 224.32721591289 +01.90868232692 14.5102 13.8748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53091_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
Preparing report for the candidate 53091_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
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Considering the candidate 53092_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53092_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:30:11.30 -03:52:46.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53110_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
Preparing report for the candidate 53110_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
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Considering the candidate 53115_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53115_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:01:43.32 -05:25:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53117_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53117_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:04:29.10 +01:48:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53119_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53119_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:58:19.34 -04:34:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.000 6337336227931454464 224.58050654112 -04.57976072757 14.3225 13.7856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53121_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53121_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:56:41.67 -02:10:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53124_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53124_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:04:50.81 -01:50:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 1.881 6339882731220872064 226.21212251060 -01.84337557328 14.4688 13.9516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.881#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53126_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53126_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:55:01.26 -04:19:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 2.023 6337602687702411776 223.75565100830 -04.31760525166 14.5067 13.7141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53128_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
Preparing report for the candidate 53128_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
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Considering the candidate 53130_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53130_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:55:04.61 +02:35:01.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)
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Considering the candidate 53132_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53132_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:55:01.65 -03:39:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 0.603 6339187187037370752 223.75699037591 -03.65423266519 14.2940 13.4404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53134_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53134_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:03:15.02 -06:48:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 3.762 6333027825977933440 225.81201483385 -06.81425944393 14.9096 14.3626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53136_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53136_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:50:20.76 -04:37:24.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)
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Considering the candidate 53138_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53138_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:01:44.61 +02:36:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.019 1153867054542883456 225.43613098269 +02.60787866578 14.5352 13.8923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53139_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53139_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:16:07.65 -02:43:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 2.482 3646202869508194944 214.03256493487 -02.72369928535 14.6869 14.3184 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53140_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53140_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:02:53.70 -05:55:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53141_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53141_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:01:35.50 +02:49:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 2.717 1154648944749023360 225.39856630002 +02.83257992330 14.3924 13.9157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53145_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53145_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:56:51.39 +02:16:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 2.503 1154220788049189120 224.21469518384 +02.27712928827 15.2028 14.5824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53147_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53147_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:58:53.64 -03:43:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 0.527 6339136678222087424 224.72336732454 -03.72449335200 14.5487 13.9198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53153_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53153_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:56:02.96 +00:20:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 1.356 3651000760294839296 224.01270329472 +00.34157120076 14.4644 13.8394 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53156_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53156_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:04:55.32 +00:43:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53157_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53157_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:57:57.80 +00:33:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 0.689 1153011325258726272 224.49102226775 +00.55991925868 14.5099 13.9540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53158_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53158_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:54:47.21 +03:00:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53162_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53162_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:00:57.68 -04:05:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.825 6338876643721878400 225.24043580204 -04.08926700171 14.3863 13.8301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53165_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53165_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:01:58.13 +01:58:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53176_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53176_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:53:26.68 -04:20:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 4.420 6337623024371507200 223.36233261072 -04.34952221509 14.4928 13.9495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53177_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53177_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:02:52.43 +01:44:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.464 1153202468483396224 225.71878331054 +01.73527248481 14.4661 13.8131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53184_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53184_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:49:48.29 -06:32:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.087 6336621407934221056 222.45100466726 -06.54427956546 14.5581 14.0520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53185_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53185_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:00:25.22 -06:45:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53187_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53187_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:55:01.72 -01:03:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 1.348 6340883492960515968 223.75753486615 -01.06298655638 14.4794 13.8862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53189_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53189_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:43:26.26 -06:56:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 1.357 6330807705842714240 220.85977251363 -06.93822981741 14.4192 13.7385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53194_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53194_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:01:32.99 -06:46:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 1.240 6333786935677468928 225.38777327064 -06.77074432923 14.5945 14.0235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53202_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53202_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:02:51.76 -01:07:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.708 6340752513637897344 225.71571342304 -01.11691333021 14.5160 14.0198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53203_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53203_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:04:07.32 +03:04:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53216_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53216_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:58:40.41 +01:59:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 1.284 1153447900094507008 224.66843280681 +01.99909251229 14.5577 13.9672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53219_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53219_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:52:53.53 -06:15:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 1.522 6336740876744497920 223.22345812885 -06.25435849685 14.2947 13.4648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53241_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53241_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:40:58.25 +02:11:07.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)
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Considering the candidate 53245_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53245_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:02:40.46 -06:09:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.146 6333922003809034624 225.66875368599 -06.15686940367 14.4634 13.8683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53249_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53249_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:03:40.24 -05:46:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 1.675 6334005566692861952 225.91813433521 -05.77719760206 14.5230 14.0200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53253_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53253_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:04:00.82 -05:43:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.092 6333960452356385152 226.00344585902 -05.72533705743 14.4868 13.9109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53287_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53287_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:04:02.71 -00:46:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.700 4419232455199560960 226.01081982472 -00.76936661044 14.7082 14.1675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53289_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53289_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:01:32.46 -06:53:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 0.763 6333034216889195904 225.38535647420 -06.89954470621 14.4831 13.9606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53291_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53291_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:30:24.04 -06:13:04.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)
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Considering the candidate 53298_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53298_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:05:43.07 -05:32:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.575 3643872282814593792 211.42929908085 -05.54279832922 14.5520 13.9627 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53299_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53299_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 15:01:21.94 -06:01:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 1.106 6333969351528538624 225.34140401896 -06.02724849470 14.4898 13.9696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53307_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 53307_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks
**** FOUND 14:09:05.79 +01:16:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.327 3667057478350772992 212.27421701163 +01.28107914792 14.4664 13.8757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 10979_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
Preparing report for the candidate 10979_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
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Considering the candidate 15232_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429
The candidate 15232_fd_Vir-09-Q1b1x1_2026-02-22_02-57-54_20.00sec_-15.00C_LIGHT_0429 did not pass the final checks