This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.1306* 03 43 55.62 +19 35 13.2 7.4 U Tau 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,2461126.6306,7.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.1306 7.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:55.62 +19:35:13.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20_00sec_-10_00C_LIGHT_0073_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20_00sec_-10_00C_LIGHT_0072_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20_00sec_-10_00C_LIGHT_0073_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20_00sec_-10_00C_LIGHT_0072_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 27.1306* 03 43 55.61 +19 35 13.1 7.5 U Tau 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,2461126.6306,7.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.1306 7.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:55.61 +19:35:13.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20_00sec_-10_00C_LIGHT_0073_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20_00sec_-10_00C_LIGHT_0072_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20_00sec_-10_00C_LIGHT_0073_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20_00sec_-10_00C_LIGHT_0072_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 27.1306* 03 48 05.03 +23 30 10.7 12.9 U Tau 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,2461126.6306,12.87,0.05,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 20260327.1306 12.87CV 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/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:05.03 +23:30:10.7 ;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_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20_00sec_-10_00C_LIGHT_0073_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20_00sec_-10_00C_LIGHT_0072_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20_00sec_-10_00C_LIGHT_0073_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20_00sec_-10_00C_LIGHT_0072_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 27.1306* 03 49 37.12 +20 58 23.3 13.6 U Tau 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,2461126.6306,13.57,0.05,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 20260327.1306 13.57CV 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/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:37.12 +20:58:23.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20_00sec_-10_00C_LIGHT_0073_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20_00sec_-10_00C_LIGHT_0072_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20_00sec_-10_00C_LIGHT_0073_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20_00sec_-10_00C_LIGHT_0072_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 27.1306* 03 34 06.35 +24 38 10.4 14.0 U Tau 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,2461126.6306,13.99,0.05,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 20260327.1306 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:34:06.35 +24:38:10.4 ;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_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20_00sec_-10_00C_LIGHT_0073_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20_00sec_-10_00C_LIGHT_0072_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20_00sec_-10_00C_LIGHT_0073_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20_00sec_-14_90C_LIGHT_0145_fits__*pix.png resample_wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20_00sec_-10_00C_LIGHT_0072_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: 2461049.67777097 09.01.2026 04:15:49.412 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
First image: 2461049.67777097 09.01.2026 04:15:49.412 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Last image: 2461126.63090003 27.03.2026 03:08:19.763 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 15
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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): 9221
Objects passed selection criteria: 9195
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 6736.25
Average stars matched: 6606.5 (98.0739 %)
Memory usage VmPeak: 115552 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 Thu Mar 26 22:17:32 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: 2461049.67777097 09.01.2026 04:15:49.412 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
First image: 2461049.67777097 09.01.2026 04:15:49.412 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Last image: 2461126.63090003 27.03.2026 03:08:19.763 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 126
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.20
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: 12 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): 58100
Objects passed selection criteria: 57941
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 44113.2
Average stars matched: 42590.8 (96.5487 %)
Memory usage VmPeak: 161360 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 Thu Mar 26 22:18:31 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/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
SExtractor catalog cache: saved Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat to cache
SExtractor catalog cache: saved Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.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: 2461126.63033476
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits exists and is non-empty
Saving wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits to local_wcs_cache/
'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits' -> 'local_wcs_cache/wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits'
wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits exists and is non-empty
Saving wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits to local_wcs_cache/
'wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits' -> 'local_wcs_cache/wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits'
wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits exists and is non-empty
Saving wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits to local_wcs_cache/
'wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits' -> 'local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits'
wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits exists and is non-empty
Saving wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits to local_wcs_cache/
'wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits' -> 'local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:41:33.240 +21:59:53.22
Second-epoch image center 03:41:26.202 +21:56:30.16
Angular distance between the image centers 0.06 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 03:41:33.240 +21:59:53.22
Second-epoch image center 03:41:23.804 +21:56:47.97
Angular distance between the image centers 0.06 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 03:41:26.202 +21:56:30.16
Second-epoch second image center 03:41:23.804 +21:56:47.97
Angular distance between the image centers 0.01051 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/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits &> /tmp/tmp.Qvdp4lmeza
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits &> /tmp/tmp.u7RzkZeeXz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits &> /tmp/tmp.NUwHFjvVc8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits &> /tmp/tmp.6cTSvRQd97
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat
Found non-empty wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat
The reference image (wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits) and catalog (wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat) found
'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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 5149 out of 11324 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.926332
a=0.000000 b=1.000000 c=22.926332
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
2.0 pix Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
2.5 pix fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
2.5 pix fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
Limiting magnitude estimates:
15.4 mag. Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
15.4 mag. Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
13.9 mag. fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
13.9 mag. fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Qvdp4lmeza (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits' -> 'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=882, passed=11324
Got 11324 stars (including 10422 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat
util/solve_plate_with_UCAC5 got 11324 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 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_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits -region wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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.u7RzkZeeXz (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits' -> 'wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=893, passed=11315
Got 11315 stars (including 10408 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat
util/solve_plate_with_UCAC5 got 11315 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 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_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits -region wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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.NUwHFjvVc8 (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_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.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_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=330, passed=4423
Got 4423 stars (including 4088 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits.cat
util/solve_plate_with_UCAC5 got 4423 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 963 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: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits -region wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.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.6cTSvRQd97 (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_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.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_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=286, passed=4451
Got 4451 stars (including 4159 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits.cat
util/solve_plate_with_UCAC5 got 4451 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 962 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: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits -region wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.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_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits'
Saving fully-calibrated image wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits'
Saving fully-calibrated image wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits'
Saving fully-calibrated image wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits'
Preparing the HTML report for the field Tau-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20503.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20482_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 20482_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:16:21.02 +19:09:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 1.528 59236296321419904 049.08801637281 +19.15355800553 10.9869 10.4697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20483_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
Preparing report for the candidate 20483_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20503_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 20503_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:15:53.44 +17:50:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 0.393 55718885608919424 048.97261984558 +17.83701622697 10.8263 10.3383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Tau-02-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/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
SExtractor catalog cache: saved Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat to cache
SExtractor catalog cache: saved Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Creating symlink local_wcs_cache/wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.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_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits exists and is non-empty
wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits exists and is non-empty
wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits exists and is non-empty
wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:41:33.240 +21:59:53.22
Second-epoch image center 03:41:26.202 +21:56:30.16
Angular distance between the image centers 0.06 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 03:41:33.240 +21:59:53.22
Second-epoch image center 03:41:23.804 +21:56:47.97
Angular distance between the image centers 0.06 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 03:41:26.202 +21:56:30.16
Second-epoch second image center 03:41:23.804 +21:56:47.97
Angular distance between the image centers 0.01051 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/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits &> /tmp/tmp.bW2LPx17kX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits &> /tmp/tmp.ejl6rIlDdT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits &> /tmp/tmp.NX1zHejyt2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits &> /tmp/tmp.4c7kxPwy2Z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat
Found non-empty wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat
The reference image (wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits) and catalog (wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat) found
'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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 5199 out of 71179 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.796402
a=0.000000 b=1.000000 c=22.796402
From vast_summary.log: estimated ref. image limiting mag.: -7.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.60
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 47 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
1.9 pix Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
2.2 pix fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
2.4 pix fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
Limiting magnitude estimates:
15.6 mag. Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
15.6 mag. Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
14.2 mag. fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
14.1 mag. fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.bW2LPx17kX (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits' -> 'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=4312, passed=71155
Got 71155 stars (including 66722 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat
util/solve_plate_with_UCAC5 got 71155 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 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_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits -region wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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.ejl6rIlDdT (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits' -> 'wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=4374, passed=71479
Got 71479 stars (including 66987 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat
util/solve_plate_with_UCAC5 got 71479 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 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_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits -region wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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.NX1zHejyt2 (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_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.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_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1419, passed=28902
Got 28902 stars (including 27442 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits.cat
util/solve_plate_with_UCAC5 got 28902 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 964 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: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits -region wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.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.4c7kxPwy2Z (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_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.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_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits.cat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1245, passed=27522
Got 27522 stars (including 26238 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits.cat
util/solve_plate_with_UCAC5 got 27522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 963 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: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits -region wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.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_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Saving fully-calibrated image wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Saving fully-calibrated image wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.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_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-07-30_20.00sec_-10.00C_LIGHT_0072.fits
Saving fully-calibrated image wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.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_2026-03-26_CI_Tau-02-Q2b1x1_221435_TTUQ2b1x1_23003_2lrjhn1d/wcs_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073.fits
Preparing the HTML report for the field Tau-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out86334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out86454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86845.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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86334_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86334_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:32:24.00 +20:37:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.672 58307312076487552 053.10023585471 +20.61945869115 13.7452 13.0078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86343_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86343_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 04:09:23.97 +18:38:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.416 47184613793110144 062.35116560554 +18.63637806206 12.4226 11.6434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86350_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86350_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:20:53.09 +18:35:35.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86351_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86351_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:16:48.98 +20:06:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 0.932 59614042989275264 049.20419262045 +20.10773755273 12.3643 11.8859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86353_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86353_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:21:05.87 +17:40:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 0.838 55830451680142464 050.27462124804 +17.67456238202 11.2770 10.9513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86354_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86354_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:16:21.03 +19:09:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 1.392 59236296321419904 049.08801637281 +19.15355800553 10.9869 10.4697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86355_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
Preparing report for the candidate 86355_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86370_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86370_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:16:13.08 +17:58:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.84, MAG_FAINT_SEARCH_LIMIT=11.82)GAIADR2_OUTPUT=# 0.480 55721947921308800 049.05438836106 +17.96986384481 10.5267 9.8548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86376_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86376_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:15:53.43 +17:50:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 0.359 55718885608919424 048.97261984558 +17.83701622697 10.8263 10.3383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86377_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86377_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:16:02.13 +17:58:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.16, MAG_FAINT_SEARCH_LIMIT=12.14)GAIADR2_OUTPUT=# 0.731 55722355942492160 049.00870106427 +17.97188208042 10.8639 10.1883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86422_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86422_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:49:07.49 +24:00:39.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86423_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86423_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:16:21.23 +17:49:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 0.896 55715415275344512 049.08868189179 +17.82687120379 12.3298 11.8658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86432_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86432_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:21:09.99 +17:40:36.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86433_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86433_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:31:40.52 +18:47:35.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86435_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86435_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:39:54.68 +25:11:45.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86437_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86437_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:45:54.11 +23:08:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.752 64955955810771840 056.47596638940 +23.14280276239 12.7280 12.1464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86447_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86447_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:16:17.97 +17:44:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 0.885 55702667812413440 049.07505295142 +17.74178917988 12.7350 12.1785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86454_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
Preparing report for the candidate 86454_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86460_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86460_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:15:44.59 +17:59:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.243 58725195213270144 048.93573793233 +17.99840052163 12.8755 12.3681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86509_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86509_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:27:02.57 +24:51:01.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86510_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86510_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:17:40.39 +17:39:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 0.490 55651540521725568 049.41821830258 +17.66206123399 12.7056 12.1626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86527_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86527_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:16:57.45 +17:38:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 0.799 55697689946090368 049.23934191133 +17.64338629702 12.6961 12.1654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86531_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86531_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:16:39.84 +17:41:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.621 55698441564596608 049.16552803261 +17.68696577028 12.7922 11.9908 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86534_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86534_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:53:56.11 +23:09:24.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86586_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86586_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 04:00:43.16 +18:12:29.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86590_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86590_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:15:40.08 +17:44:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.011 55691780071030272 048.91723118634 +17.74984090398 12.7428 12.1858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.011#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86595_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86595_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:34:24.15 +22:45:55.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86598_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86598_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:42:50.29 +24:29:29.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86614_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86614_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:36:51.41 +23:11:58.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86634_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86634_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:45:01.24 +24:05:32.7 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86648_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86648_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:31:22.91 +26:10:22.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86656_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86656_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:24:28.62 +22:02:25.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86657_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86657_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:51:23.54 +24:31:30.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86663_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86663_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:33:55.27 +24:15:33.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86675_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86675_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:44:11.38 +25:53:40.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86681_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86681_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:37:23.87 +18:13:51.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86695_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86695_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:28:55.69 +25:00:16.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86708_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86708_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:16:40.75 +17:39:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.003 55698067903215488 049.17008354652 +17.65553997503 13.2800 12.6994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.003#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86747_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86747_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:42:11.27 +22:47:53.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86753_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86753_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:30:04.05 +24:10:21.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86766_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86766_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:41:23.14 +24:59:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86780_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86780_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:15:55.72 +18:14:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 0.663 58737702158018816 048.98214953766 +18.23743341836 13.4345 12.9246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86790_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86790_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:38:17.71 +25:04:06.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86796_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
Preparing report for the candidate 86796_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86798_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 86798_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks
**** FOUND 03:36:27.89 +23:53:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.927 67834614690074752 054.11661108032 +23.89330596126 13.6412 12.7597 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86845_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
Preparing report for the candidate 86845_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63847_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073
The candidate 63847_fd_Tau-02-Q2b1x1_2026-03-26_22-08-19_20.00sec_-10.00C_LIGHT_0073 did not pass the final checks