This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ
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!
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,2461126.9219,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.4219 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:39:48.45 -11:54:58.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20_00sec_-14_90C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20_00sec_-14_90C_LIGHT_0460_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20_00sec_-14_90C_LIGHT_0460_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!
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,2461126.9219,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.4219 13.67CV 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/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:54:44.69 -11:54:05.0 ;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_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20_00sec_-14_90C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20_00sec_-14_90C_LIGHT_0460_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20_00sec_-14_90C_LIGHT_0460_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.4219* 14 19 54.05 -08 52 58.7 13.8 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461126.9219,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.4219 13.75CV 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/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:19:54.05 -08:52:58.7 ;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_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20_00sec_-14_90C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20_00sec_-14_90C_LIGHT_0460_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20_00sec_-14_90C_LIGHT_0460_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!
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,2461126.9219,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.4219 13.85CV 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/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:23:46.47 -11:09:36.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20_00sec_-14_90C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20_00sec_-14_90C_LIGHT_0460_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20_00sec_-14_90C_LIGHT_0460_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.4219* 14 26 13.48 -07 25 09.4 14.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461126.9219,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.4219 14.37CV 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/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:26:13.48 -07:25:09.4 ;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_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20_00sec_-14_90C_LIGHT_0461_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20_00sec_-14_90C_LIGHT_0460_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20_00sec_-14_90C_LIGHT_0461_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20_00sec_-15_00C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20_00sec_-14_90C_LIGHT_0460_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: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
First image: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Last image: 2461126.92218171 27.03.2026 10:07:46.500 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.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.: -8.16
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5881
Objects passed selection criteria: 5872
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 4992.75
Average stars matched: 4660 (93.3353 %)
Memory usage VmPeak: 111852 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 06:19:50 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
First image: 2461098.90985984 27.02.2026 09:50:01.890 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Last image: 2461126.92218171 27.03.2026 10:07:46.500 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 124
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
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: 10 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): 32946
Objects passed selection criteria: 32889
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 28545.5
Average stars matched: 26471.8 (92.7353 %)
Memory usage VmPeak: 133360 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 06:20:27 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat to cache
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.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: 2461126.92157742
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits exists and is non-empty
Saving wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits to local_wcs_cache/
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> 'local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits exists and is non-empty
Saving wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits to local_wcs_cache/
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> 'local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits exists and is non-empty
Saving wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits to local_wcs_cache/
'wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits' -> 'local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits'
wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits exists and is non-empty
Saving wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits to local_wcs_cache/
'wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits' -> 'local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:34:09.421 -09:59:51.45
Angular distance between the image centers 0.07 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:34:10.147 -10:00:09.88
Angular distance between the image centers 0.07 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 14:34:09.421 -09:59:51.45
Second-epoch second image center 14:34:10.147 -10:00:09.88
Angular distance between the image centers 0.00592 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/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits &> /tmp/tmp.cUbVRk8s1d
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits &> /tmp/tmp.JSaY2iADaC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits &> /tmp/tmp.Zt6ncDkl18
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits &> /tmp/tmp.YU7ucrNWBC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
Found non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
The reference image (wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits) and catalog (wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat) found
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
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 3683 out of 5992 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.914760
a=0.000000 b=1.000000 c=22.914760
From vast_summary.log: estimated ref. image limiting mag.: -8.16
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.75
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.75
Magnitude calibration plot:
____ 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:
2.5 pix Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
2.4 pix Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
2.7 pix fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
2.7 pix fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
Limiting magnitude estimates:
14.8 mag. Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
14.8 mag. Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
14.6 mag. fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
14.7 mag. fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.cUbVRk8s1d (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_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> 'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=377, passed=5992
Got 5992 stars (including 5611 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 5992 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
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: 0.45"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 971 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits -region wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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.JSaY2iADaC (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_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> 'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=404, passed=5931
Got 5931 stars (including 5520 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
util/solve_plate_with_UCAC5 got 5931 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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: 0.47"
Estimated accuracy of the plate solution: 0.47"
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_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits -region wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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.Zt6ncDkl18 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=277, passed=5831
Got 5831 stars (including 5548 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits.cat
util/solve_plate_with_UCAC5 got 5831 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits -region wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.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.YU7ucrNWBC (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=283, passed=5898
Got 5898 stars (including 5613 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat
util/solve_plate_with_UCAC5 got 5898 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits -region wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
Saving fully-calibrated image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits'
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits'
Preparing the HTML report for the field Lib-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20496_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 20496_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:10:21.61 -13:18:13.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20723_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 20723_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:58:14.28 -11:30:14.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Lib-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat to cache
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Creating symlink local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.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_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits exists and is non-empty
wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits exists and is non-empty
wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits exists and is non-empty
wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:34:09.421 -09:59:51.45
Angular distance between the image centers 0.07 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:34:25.896 -10:01:24.58
Second-epoch image center 14:34:10.147 -10:00:09.88
Angular distance between the image centers 0.07 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 14:34:09.421 -09:59:51.45
Second-epoch second image center 14:34:10.147 -10:00:09.88
Angular distance between the image centers 0.00592 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/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits &> /tmp/tmp.dqetl7MjhW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits &> /tmp/tmp.UyQNPj80dp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits &> /tmp/tmp.4QGsX3a2cE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits &> /tmp/tmp.hNkwEx4Tav
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
Found non-empty wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits and wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
The reference image (wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits) and catalog (wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat) found
'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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 3887 out of 33758 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.758633
a=0.000000 b=1.000000 c=22.758633
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.89
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 82 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
2.3 pix Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
2.7 pix fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
2.8 pix fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
Limiting magnitude estimates:
14.9 mag. Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
14.9 mag. Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
14.7 mag. fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
14.7 mag. fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.dqetl7MjhW (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_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits' -> 'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1364, passed=33749
Got 33749 stars (including 32349 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 33749 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits -region wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.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.UyQNPj80dp (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_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits' -> 'wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1488, passed=34765
Got 34765 stars (including 33244 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat
util/solve_plate_with_UCAC5 got 34765 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 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: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits -region wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.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.4QGsX3a2cE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1144, passed=30131
Got 30131 stars (including 28951 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits.cat
util/solve_plate_with_UCAC5 got 30131 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 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 965 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 - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits -region wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.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.hNkwEx4Tav (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1188, passed=30389
Got 30389 stars (including 29174 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat
util/solve_plate_with_UCAC5 got 30389 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 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: 0.38"
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 967 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 - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits -region wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-01_20.00sec_-15.00C_LIGHT_0208.fits
Saving fully-calibrated image wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/wcs_Lib-01-Q2b1x1_2026-02-27_03-50-48_20.00sec_-14.90C_LIGHT_0209.fits
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-06-54_20.00sec_-14.90C_LIGHT_0460.fits
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-01-Q2b1x1_061740_TTUQ2b1x1_1361_Ho6zPyEJ/wcs_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461.fits
Preparing the HTML report for the field Lib-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53016.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57097.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57294.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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
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Considering the candidate 53005_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 53005_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:47:16.61 -13:11:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 3.665 6311575460766846208 221.81867083481 -13.19159539746 14.3815 13.8183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53009_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 53009_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:45:19.23 -12:24:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53015_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 53015_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:51:32.73 -13:49:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 0.614 6311372978828634752 222.88654635854 -13.82651016745 12.6530 11.9749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53016_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 53016_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:12:27.03 -08:27:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.094 3639223650731656576 213.11265300084 -08.46158625913 12.6544 12.1283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53233_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 53233_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:46:16.79 -11:05:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53778_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 53778_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 53910_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
Preparing report for the candidate 53910_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
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Considering the candidate 54063_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 54063_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 54132_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 54132_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:53:06.34 -11:16:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54409_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 54409_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 54668_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 54668_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 54722_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 54722_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:54:39.48 -10:20:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54809_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 54809_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 54837_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 54837_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 54941_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 54941_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 55012_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55012_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 55037_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55037_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 55062_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55062_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 55139_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55139_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 55167_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55167_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 55197_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55197_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 55329_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55329_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 55508_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55508_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 55548_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55548_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 55703_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55703_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 55754_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55754_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 55775_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55775_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 55795_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55795_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 55805_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55805_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 55825_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55825_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 55876_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
Preparing report for the candidate 55876_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
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Considering the candidate 55899_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55899_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 55900_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55900_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 55904_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55904_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 55946_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55946_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 55975_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 55975_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 56157_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56157_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 56190_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56190_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 56260_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56260_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 56278_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56278_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 56376_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
Preparing report for the candidate 56376_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
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Considering the candidate 56433_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
Preparing report for the candidate 56433_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
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Considering the candidate 56442_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56442_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 56493_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56493_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:52:08.50 -10:20:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56547_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56547_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 56588_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56588_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 56637_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56637_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 56665_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56665_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 56702_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56702_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:52:33.14 -11:37:00.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)
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Considering the candidate 56744_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56744_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 56751_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56751_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 56795_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56795_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:51:35.16 -14:00:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.854 6310526045637745664 222.89692453242 -14.00335758753 14.0321 13.4902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56805_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56805_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 56831_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56831_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 56860_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56860_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:53:11.58 -11:06:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56889_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56889_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:42:16.03 -14:10:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56915_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56915_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:51:27.34 -14:08:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 0.648 6310519723445871232 222.86380153300 -14.13816442835 14.2044 13.6460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56919_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56919_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 56941_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56941_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 56962_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56962_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:49:00.13 -13:53:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56974_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 56974_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 57046_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57046_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 57097_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57097_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:46:29.02 -14:00:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 1.719 6310944615970467968 221.62132064472 -14.01311620010 14.1710 13.4757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57179_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57179_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 57180_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57180_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:50:07.40 -12:40:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57203_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57203_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 57205_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57205_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 57216_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57216_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:47:32.53 -13:36:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 1.470 6311336282628042368 221.88594041346 -13.60798958953 14.2495 13.6005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57226_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57226_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 57238_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57238_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:48:23.86 -12:43:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 1.154 6311687095556759040 222.09911205927 -12.72070395166 14.4530 13.9237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57248_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57248_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 57250_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57250_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:46:00.27 -13:52:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57258_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57258_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:49:56.10 -09:53:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57269_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57269_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 57271_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57271_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:43:42.72 -13:30:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 1.963 6311213274764719744 220.92827137993 -13.50130075510 14.2847 13.6284 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57272_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57272_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:58:05.01 -09:37:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 2.204 6326065443472667776 224.52097454942 -09.62421533264 14.4138 13.8939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57284_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57284_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:53:43.60 -11:53:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57294_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
Preparing report for the candidate 57294_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
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Considering the candidate 57324_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57324_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:29:49.11 -13:12:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57331_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 57331_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:12:45.84 -08:25:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.131 3639244747611018240 213.19158187073 -08.42233222871 14.4283 13.7310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 25642_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 25642_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks
**** FOUND 14:42:00.63 -05:49:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05170_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461
The candidate 05170_fd_Lib-01-Q2b1x1_2026-03-27_05-07-46_20.00sec_-14.90C_LIGHT_0461 did not pass the final checks