This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS
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 22.3514* 12 00 16.65 +01 31 33.4 11.7 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.8514,11.71,0.05,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 20260222.3514 11.71CV 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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:00:16.65 +01:31:33.4 ;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-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_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 22.3514* 12 05 01.69 +04 00 19.3 13.0 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,2461093.8514,12.96,0.05,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 20260222.3514 12.96CV 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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:05:01.69 +04:00:19.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_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 22.3514* 11 40 26.19 +06 26 47.6 13.0 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,2461093.8514,13.02,0.05,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 20260222.3514 13.02CV 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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:40:26.19 +06:26:47.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_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 22.3514* 12 27 29.06 +01 11 03.6 13.0 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,2461093.8514,13.04,0.05,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 20260222.3514 13.04CV 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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:27:29.06 +01:11:03.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_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 22.3514* 11 39 23.82 +05 28 13.7 13.5 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.8514,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.3514 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:39:23.82 +05:28:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_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 22.3514* 11 41 01.19 +07 07 01.6 14.0 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,2461093.8514,13.99,0.05,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 20260222.3514 13.99CV 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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:41:01.19 +07:07:01.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_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 22.3514* 12 03 02.45 +07 10 52.1 14.3 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,2461093.8514,14.27,0.05,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 20260222.3514 14.27CV 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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:03:02.45 +07:10:52.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_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 22.3514* 12 27 35.62 +06 23 01.1 14.5 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.8514,14.47,0.05,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 20260222.3514 14.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:27:35.62 +06:23:01.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_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 22.3514* 11 43 23.56 +05 30 46.2 14.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.8514,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.3514 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:43:23.56 +05:30:46.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_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 22.3514* 12 04 39.20 +04 24 07.0 14.5 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.8514,14.50,0.05,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 20260222.3514 14.50CV 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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:04:39.20 +04:24:07.0 ;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-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20_00sec_-15_00C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20_00sec_-15_00C_LIGHT_0394_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: 2461082.88694909 11.02.2026 09:17:02.401 /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
First image: 2461082.88694909 11.02.2026 09:17:02.401 /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
Last image: 2461093.85168088 22.02.2026 08:26:15.228 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.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.: -7.64
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): 5598
Objects passed selection criteria: 5595
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: 5428.5
Average stars matched: 5218.75 (96.1361 %)
Memory usage VmPeak: 111808 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 04:14:17 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: 2461082.88694909 11.02.2026 09:17:02.401 /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
First image: 2461082.88694909 11.02.2026 09:17:02.401 /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
Last image: 2461093.85168088 22.02.2026 08:26:15.228 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 65
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
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: 21 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): 31125
Objects passed selection criteria: 31039
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: 30131.2
Average stars matched: 28913 (95.9569 %)
Memory usage VmPeak: 132836 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 04:16:39 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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
SExtractor catalog cache: saved Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat to cache
SExtractor catalog cache: saved Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.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: 2461093.85119028
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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits exists and is non-empty
Saving wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits to local_wcs_cache/
'wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits' -> 'local_wcs_cache/wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits'
wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits exists and is non-empty
Saving wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits to local_wcs_cache/
'wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits' -> 'local_wcs_cache/wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits'
wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits exists and is non-empty
Saving wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits to local_wcs_cache/
'wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits' -> 'local_wcs_cache/wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits'
wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits exists and is non-empty
Saving wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits to local_wcs_cache/
'wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits' -> 'local_wcs_cache/wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:59.751 +06:00:08.05
Second-epoch image center 12:00:19.566 +06:02:12.98
Angular distance between the image centers 0.09 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:59.751 +06:00:08.05
Second-epoch image center 12:00:19.522 +06:01:34.05
Angular distance between the image centers 0.09 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 12:00:19.566 +06:02:12.98
Second-epoch second image center 12:00:19.522 +06:01:34.05
Angular distance between the image centers 0.01081 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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits &> /tmp/tmp.pQ0PTRkXtq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits &> /tmp/tmp.VigBwsEFK5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits &> /tmp/tmp.6xSxDzcotM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits &> /tmp/tmp.6NBIUeZvIo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits and wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits and wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat
Found non-empty wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits and wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat
The reference image (wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits) and catalog (wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat) found
'wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.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 3180 out of 5240 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.855205
a=0.000000 b=1.000000 c=22.855205
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.22
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.22
____ 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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
2.1 pix Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
2.2 pix fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
2.2 pix fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
Limiting magnitude estimates:
15.2 mag. Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
15.2 mag. Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
15.3 mag. fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
15.2 mag. fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.pQ0PTRkXtq (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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits' -> 'wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
WCS_IMAGE_NAME=wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
WCS-calibrated image found: wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
Checking if the catalog wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat corresponding to the image wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits alredy exist and is non-empty...
Catalog wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat corresponding to the image wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
WCS catalog name: wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=396, passed=5240
Got 5240 stars (including 4833 good ones) from the SExtractor catalog wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat
util/solve_plate_with_UCAC5 got 5240 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits -region wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.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.VigBwsEFK5 (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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.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-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits' -> 'wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
WCS_IMAGE_NAME=wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
WCS-calibrated image found: wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
Checking if the catalog wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits.cat corresponding to the image wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits alredy exist and is non-empty...
Catalog wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits.cat corresponding to the image wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
WCS catalog name: wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=406, passed=5340
Got 5340 stars (including 4929 good ones) from the SExtractor catalog wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits.cat
util/solve_plate_with_UCAC5 got 5340 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 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: 0.37"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits -region wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.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.6xSxDzcotM (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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
WCS_IMAGE_NAME=wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
WCS-calibrated image found: wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
Checking if the catalog wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits.cat corresponding to the image wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits.cat corresponding to the image wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
WCS catalog name: wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=427, passed=5637
Got 5637 stars (including 5205 good ones) from the SExtractor catalog wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits.cat
util/solve_plate_with_UCAC5 got 5637 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits -region wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.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.6NBIUeZvIo (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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
WCS_IMAGE_NAME=wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
WCS-calibrated image found: wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
Checking if the catalog wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits.cat corresponding to the image wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits.cat corresponding to the image wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
WCS catalog name: wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.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=5640
Got 5640 stars (including 5217 good ones) from the SExtractor catalog wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits.cat
util/solve_plate_with_UCAC5 got 5640 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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 973 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 - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits -region wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.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-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits'
Saving fully-calibrated image wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits'
Preparing the HTML report for the field Vir-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20325.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
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 20325_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
Preparing report for the candidate 20325_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20342_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
The candidate 20342_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395 did not pass the final checks
**** FOUND 11:55:21.94 +03:48:15.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 14s
Prepared the HTML report for the field Vir-02-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 ####
12:00:16.65 +01:31:33.4
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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
SExtractor catalog cache: saved Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat to cache
SExtractor catalog cache: saved Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
Creating symlink local_wcs_cache/wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits exists and is non-empty
wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits exists and is non-empty
wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits exists and is non-empty
wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:59:59.751 +06:00:08.05
Second-epoch image center 12:00:19.566 +06:02:12.98
Angular distance between the image centers 0.09 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:59.751 +06:00:08.05
Second-epoch image center 12:00:19.522 +06:01:34.05
Angular distance between the image centers 0.09 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 12:00:19.566 +06:02:12.98
Second-epoch second image center 12:00:19.522 +06:01:34.05
Angular distance between the image centers 0.01081 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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits &> /tmp/tmp.03rAkILRUl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits &> /tmp/tmp.gNy8N7Dlqw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits &> /tmp/tmp.oVMp2rE9y8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits &> /tmp/tmp.7uURaEjqTl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits and wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits and wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat
Found non-empty wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits and wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat
The reference image (wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits) and catalog (wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat) found
'wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.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 3254 out of 29928 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.738346
a=0.000000 b=1.000000 c=22.738346
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 14 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
1.9 pix Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
2.0 pix fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
2.1 pix fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
Limiting magnitude estimates:
15.4 mag. Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
15.4 mag. Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
15.4 mag. fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
15.4 mag. fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.03rAkILRUl (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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.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-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits' -> 'wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
WCS_IMAGE_NAME=wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
WCS-calibrated image found: wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
Checking if the catalog wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat corresponding to the image wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits alredy exist and is non-empty...
Catalog wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat corresponding to the image wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits
WCS catalog name: wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=1068, passed=29906
Got 29906 stars (including 28785 good ones) from the SExtractor catalog wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat
util/solve_plate_with_UCAC5 got 29906 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 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 973 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 - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits -region wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-02_20.00sec_-15.00C_LIGHT_0425.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.gNy8N7Dlqw (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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.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-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits' -> 'wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
WCS_IMAGE_NAME=wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
WCS-calibrated image found: wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
Checking if the catalog wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits.cat corresponding to the image wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits alredy exist and is non-empty...
Catalog wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits.cat corresponding to the image wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits
WCS catalog name: wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1115, passed=30307
Got 30307 stars (including 29142 good ones) from the SExtractor catalog wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits.cat
util/solve_plate_with_UCAC5 got 30307 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits -region wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-02-Q1b1x1_2026-02-11_03-17-58_20.00sec_-14.90C_LIGHT_0426.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.oVMp2rE9y8 (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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
WCS_IMAGE_NAME=wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
WCS-calibrated image found: wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
Checking if the catalog wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits.cat corresponding to the image wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits.cat corresponding to the image wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
WCS catalog name: wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1247, passed=30674
Got 30674 stars (including 29363 good ones) from the SExtractor catalog wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits.cat
util/solve_plate_with_UCAC5 got 30674 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits -region wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.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.7uURaEjqTl (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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
WCS_IMAGE_NAME=wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
WCS-calibrated image found: wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
Checking if the catalog wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits.cat corresponding to the image wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits.cat corresponding to the image wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
WCS catalog name: wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1207, passed=30572
Got 30572 stars (including 29306 good ones) from the SExtractor catalog wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits.cat
util/solve_plate_with_UCAC5 got 30572 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-22_CI_Vir-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits -region wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.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-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-25-32_20.00sec_-15.00C_LIGHT_0394.fits
Saving fully-calibrated image wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.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-02-Q1b1x1_022651_TTUQ1b1x1_24877_Fl2d9QUS/wcs_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395.fits
Preparing the HTML report for the field Vir-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out32368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out32437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32586.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 7s
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Considering the candidate 32368_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
The candidate 32368_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395 did not pass the final checks
**** FOUND 12:15:59.55 +05:51:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.262 3895229918053535232 183.99811418485 +05.85501063855 14.6060 13.9881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32396_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
The candidate 32396_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395 did not pass the final checks
**** FOUND 12:00:16.66 +01:31:33.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 32437_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
Preparing report for the candidate 32437_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
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Considering the candidate 32438_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
Preparing report for the candidate 32438_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
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Considering the candidate 32439_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
Preparing report for the candidate 32439_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
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Considering the candidate 32464_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
Preparing report for the candidate 32464_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
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Considering the candidate 32500_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
Preparing report for the candidate 32500_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
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Considering the candidate 32506_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
The candidate 32506_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395 did not pass the final checks
**** FOUND 12:19:12.14 +09:22:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32513_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
The candidate 32513_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395 did not pass the final checks
**** FOUND 12:07:58.14 +00:59:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 2.643 3699450808892193152 181.99171356650 +00.99124867352 14.1446 13.4496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32514_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
Preparing report for the candidate 32514_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
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Considering the candidate 32534_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
Preparing report for the candidate 32534_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
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Considering the candidate 32542_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395
The candidate 32542_fd_Vir-02-Q1b1x1_2026-02-22_02-26-15_20.00sec_-15.00C_LIGHT_0395 did not pass the final checks