This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2132* 05 46 02.80 +23 20 15.3 11.5 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,2461121.7132,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2132 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:02.80 +23:20:15.3 ;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-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2132* 05 12 10.05 +20 36 21.3 11.4 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,2461121.7132,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2132 11.41CV 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:10.05 +20:36:21.3 ;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-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2132* 05 06 55.91 +25 45 04.9 12.3 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,2461121.7132,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2132 12.26CV 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:06:55.91 +25:45:04.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2132* 05 07 52.26 +18 13 13.4 12.7 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,2461121.7132,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2132 12.68CV 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:52.26 +18:13:13.4 ;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-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2132* 05 05 25.90 +21 58 39.9 12.8 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,2461121.7132,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2132 12.82CV 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:05:25.90 +21:58:39.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2132* 05 17 23.72 +19 07 24.3 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,2461121.7132,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2132 13.63CV 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:23.72 +19:07:24.3 ;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-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2132* 05 14 28.79 +23 32 59.0 14.1 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,2461121.7132,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2132 14.05CV 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:14:28.79 +23:32:59.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2132* 05 33 43.66 +21 07 37.3 14.5 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,2461121.7132,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2132 14.46CV 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:33:43.66 +21:07:37.3 ;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-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2132* 05 35 39.98 +25 20 18.2 14.7 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,2461121.7132,14.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2132 14.70CV 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:35:39.98 +25:20:18.2 ;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-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2132* 05 13 57.67 +19 10 11.4 14.8 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,2461121.7132,14.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2132 14.76CV 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:57.67 +19:10:11.4 ;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-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2132* 05 22 21.64 +18 21 17.2 12.8 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,2461121.7132,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2132 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:22:21.64 +18:21:17.2 ;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-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20_00sec_-15_00C_LIGHT_0041_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: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
First image: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Last image: 2461121.71345718 22.03.2026 05:07:12.700 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 18
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
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: 11 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): 21976
Objects passed selection criteria: 21962
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 21005.8
Average stars matched: 20579.8 (97.972 %)
Memory usage VmPeak: 126084 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 01:40:48 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: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
First image: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Last image: 2461121.71345718 22.03.2026 05:07:12.700 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 169
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
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: 93 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): 156722
Objects passed selection criteria: 156427
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 145122
Average stars matched: 140752 (96.9891 %)
Memory usage VmPeak: 2570576 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 01:44:09 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
SExtractor catalog cache: saved Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461121.71298353
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits exists and is non-empty
Saving wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits to local_wcs_cache/
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'local_wcs_cache/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits exists and is non-empty
Saving wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits to local_wcs_cache/
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> 'local_wcs_cache/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits'
wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits'
wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.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 05:32:19.563 +21:59:58.39
Second-epoch image center 05:32:18.736 +21:59:58.91
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:32:19.563 +21:59:58.39
Second-epoch image center 05:32:17.192 +22:00:01.83
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:32:18.736 +21:59:58.91
Second-epoch second image center 05:32:17.192 +22:00:01.83
Angular distance between the image centers 0.00602 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits &> /tmp/tmp.oYFeIuTcD7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits &> /tmp/tmp.G2W6eKTMVB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.JHRn2GVVFF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.FpQkwYdM4C
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
Found non-empty wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
The reference image (wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits) and catalog (wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat) found
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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 10157 out of 22997 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.956266
a=0.000000 b=1.000000 c=22.956266
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 17 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
2.0 pix Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
2.2 pix fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
2.2 pix fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
Limiting magnitude estimates:
15.3 mag. Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
15.3 mag. Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
15.0 mag. fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
15.0 mag. fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.1 (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.oYFeIuTcD7 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2479, passed=22997
Got 22997 stars (including 20487 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
util/solve_plate_with_UCAC5 got 22997 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -region wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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.G2W6eKTMVB (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> 'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2545, passed=22806
Got 22806 stars (including 20234 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat
util/solve_plate_with_UCAC5 got 22806 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 934.0'
Seting catalog search parameters based on the expected field of view 934.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012972 (46.7 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010378 (37.4 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 616 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: 2.04"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.53"
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 661 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.45"
Estimated accuracy of the plate solution: 1.58"
Excluding outliers - 624 stars left (next iteration limit 630)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits -region wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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.JHRn2GVVFF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1581, passed=19459
Got 19459 stars (including 17860 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 19459 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.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.FpQkwYdM4C (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1536, passed=19241
Got 19241 stars (including 17685 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 19241 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 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: 0.40"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
Saving fully-calibrated image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits'
Preparing the HTML report for the field Tau-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out31441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31486.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: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31430_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 31430_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:44:17.58 +22:41:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31441_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
Preparing report for the candidate 31441_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31442_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
Preparing report for the candidate 31442_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31452_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 31452_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:02:40.11 +22:14:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31454_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 31454_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:47:46.40 +23:58:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31457_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 31457_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:30:44.17 +20:13:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 1.374 3401302215087738624 082.68398545729 +20.23312788265 11.9649 11.4175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31460_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 31460_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:45:01.08 +26:19:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31461_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 31461_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:15:47.36 +26:45:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31463_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 31463_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:49:09.60 +25:07:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31466_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 31466_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:46:41.41 +20:36:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31473_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 31473_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:34:14.62 +23:02:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31478_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 31478_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:31:11.86 +22:43:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31486_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
Preparing report for the candidate 31486_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31494_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 31494_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:45:39.16 +18:56:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 1.176 3399237091731720576 086.41312609870 +18.94876891923 12.2323 11.7384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31498_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 31498_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:27:24.08 +22:55:59.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31502_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 31502_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:27:59.33 +20:26:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14186_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 14186_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:55:48.82 +20:10:31.2 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Tau-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:46:02.80 +23:20:15.3
05:12:10.05 +20:36:21.3
05:06:55.91 +25:45:04.9
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
SExtractor catalog cache: saved Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Creating symlink local_wcs_cache/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits exists and is non-empty
wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits exists and is non-empty
wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.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 05:32:19.563 +21:59:58.39
Second-epoch image center 05:32:18.736 +21:59:58.91
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:32:19.563 +21:59:58.39
Second-epoch image center 05:32:17.192 +22:00:01.83
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:32:18.736 +21:59:58.91
Second-epoch second image center 05:32:17.192 +22:00:01.83
Angular distance between the image centers 0.00602 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits &> /tmp/tmp.C4QoySCHmZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits &> /tmp/tmp.ZngR9Lhzh7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.wkOSc8RKOM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.4khyWE5dsz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
Found non-empty wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
The reference image (wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits) and catalog (wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat) found
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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 10499 out of 167968 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.793970
a=0.000000 b=1.000000 c=22.793970
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 151 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
1.9 pix Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
2.3 pix fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
2.2 pix fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
Limiting magnitude estimates:
15.5 mag. Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
15.5 mag. Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
15.1 mag. fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
15.1 mag. fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.C4QoySCHmZ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=21684, passed=167940
Got 167940 stars (including 145994 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
util/solve_plate_with_UCAC5 got 167940 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 933 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: 0.37"
Excluding outliers - 932 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -region wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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.ZngR9Lhzh7 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> 'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=50, blended=21854, passed=169419
Got 169419 stars (including 147299 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat
util/solve_plate_with_UCAC5 got 169419 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 934.0'
Seting catalog search parameters based on the expected field of view 934.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012972 (46.7 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010378 (37.4 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 589 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: 2.15"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.75"
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 643 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.74"
Estimated accuracy of the plate solution: 1.56"
Excluding outliers - 601 stars left (next iteration limit 606)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits -region wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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.wkOSc8RKOM (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=12818, passed=122693
Got 122693 stars (including 109703 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 122693 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 929 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.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.4khyWE5dsz (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=12953, passed=123807
Got 123807 stars (including 110646 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 123807 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Saving fully-calibrated image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-06-31_20.00sec_-15.00C_LIGHT_0041.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_000756_TTUQ1b1x1_10090_BADpc6NQ/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042.fits
Preparing the HTML report for the field Tau-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out193688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193714.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193921.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194154.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194291.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out126539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194529.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
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: 5s
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Considering the candidate 193658_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193658_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193673_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193673_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:03:12.55 +25:18:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193688_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193688_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:10:32.48 +18:15:38.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)
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Considering the candidate 193691_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193691_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:55:59.84 +17:23:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 2.751 3350012166614136320 089.00006624972 +17.39553000054 14.4550 13.9217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193701_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193701_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:42:14.08 +25:29:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193703_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193703_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:38:39.84 +17:39:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.093 3397465950298969728 084.66579137320 +17.66384043060 13.6983 12.8494 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.093#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193705_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193705_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:55:08.31 +22:19:32.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)
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Considering the candidate 193706_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193706_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:22:01.37 +20:10:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.283 3401827923380735104 080.50532857727 +20.17630159793 13.8414 13.2112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193708_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193708_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:36:19.06 +24:13:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 1.164 3404684931330404480 084.07920460828 +24.23256455540 13.4496 12.4156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193710_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193710_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:30:48.44 +20:15:50.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)
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Considering the candidate 193711_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193711_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:40:28.75 +26:30:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193713_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193713_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:04:03.80 +26:13:08.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)
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Considering the candidate 193714_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193714_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:40:00.25 +26:22:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.852 3441027226603659392 085.00102700359 +26.38198663498 14.0663 13.4052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193715_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193715_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:56:25.79 +18:57:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193730_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193730_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:04:54.73 +26:09:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193748_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193748_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:46:02.74 +23:20:16.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 193749_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193749_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:12:10.07 +20:36:21.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 193760_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193760_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 193766_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193766_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:41:56.14 +22:38:54.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193767_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193767_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:06:55.91 +25:45:05.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 193790_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193790_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:05:46.02 +26:25:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193792_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193792_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:43:34.70 +25:27:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193795_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193795_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:04:13.43 +25:24:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193796_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193796_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 193799_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
Preparing report for the candidate 193799_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
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Considering the candidate 193803_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193803_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:31:11.00 +20:10:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193809_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193809_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:05:41.78 +23:02:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193813_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
Preparing report for the candidate 193813_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
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Considering the candidate 193816_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193816_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 193817_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193817_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:29:17.26 +18:20:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193825_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193825_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:48:27.20 +20:53:27.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193845_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193845_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:58:09.53 +21:58:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193846_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193846_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:49:44.95 +24:06:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193857_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193857_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:55:14.60 +20:28:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193858_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193858_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:10:48.65 +25:09:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193861_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193861_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:52:52.90 +17:05:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193862_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193862_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:41:53.54 +18:32:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193867_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193867_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:39:27.67 +21:47:28.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193873_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193873_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:51:41.47 +23:14:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193877_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193877_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:20:20.48 +25:08:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193887_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193887_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:49:11.96 +19:49:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193888_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193888_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:24:45.92 +17:11:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.616 3394235451993572480 081.19088173291 +17.19142993815 13.0314 12.1088 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193898_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193898_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:59:41.59 +19:52:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193904_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193904_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:08:15.93 +20:40:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193910_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193910_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:43:36.71 +25:27:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193912_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193912_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:41:10.45 +27:03:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193921_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193921_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:56:32.22 +18:25:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.179 3350520244064706304 089.13394627528 +18.42235013222 13.8824 13.2615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193923_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193923_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:27:21.81 +17:17:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193926_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193926_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:36:40.74 +18:53:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193928_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193928_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:58:05.53 +24:37:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193930_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193930_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:50:27.71 +18:02:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193931_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193931_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:47:20.98 +23:52:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193932_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193932_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:48:40.40 +18:15:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193934_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193934_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:17:30.41 +20:09:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193937_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193937_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:57:16.87 +22:22:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.652 3424134437328421760 089.32063409725 +22.37394336021 13.9322 13.3490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193938_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
Preparing report for the candidate 193938_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
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Considering the candidate 193941_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193941_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:54:24.84 +18:35:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193945_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193945_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:57:10.53 +21:28:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193969_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193969_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:03:16.08 +16:56:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193983_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193983_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:54:42.44 +17:25:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193987_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193987_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:51:36.83 +16:46:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193994_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 193994_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:01:09.84 +22:31:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194001_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194001_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:36:30.62 +25:57:49.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194002_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194002_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:22:01.85 +18:15:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194003_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194003_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 194008_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194008_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:27:58.66 +21:26:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194013_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194013_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:27:39.37 +21:58:01.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194025_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194025_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:47:31.26 +17:37:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194035_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194035_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:32:03.00 +19:09:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194043_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194043_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 194046_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194046_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:31:04.94 +23:13:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194047_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194047_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 194050_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194050_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:25:45.04 +22:11:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 4.665 3415986231533160704 081.43794406315 +22.19329781638 14.2891 13.5691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194055_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
Preparing report for the candidate 194055_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
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Considering the candidate 194057_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194057_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:46:04.92 +19:23:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194069_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194069_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:54:10.39 +24:05:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194077_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194077_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:20:18.66 +23:09:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194078_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194078_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:55:51.34 +23:58:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194081_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194081_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 194088_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194088_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 194092_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194092_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:07:49.14 +24:05:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194093_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194093_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:39:50.12 +19:23:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194094_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194094_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 194101_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194101_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:34:19.97 +20:16:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194104_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194104_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:02:10.39 +23:35:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194106_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194106_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 194112_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194112_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:31:18.42 +19:54:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 2.533 3401228895702932736 082.82749139725 +19.91159536668 14.4304 13.8114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194133_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194133_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:44:15.47 +24:09:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194142_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194142_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:20:42.13 +22:49:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 3.031 3414822810791381888 080.17494159819 +22.81755972688 14.0542 12.9594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194144_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194144_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 194147_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194147_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:38:24.17 +26:07:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194153_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194153_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 194154_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194154_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:57:02.25 +26:30:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 1.019 3429912267854385152 089.25915878524 +26.50517873188 14.5038 13.8571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194158_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194158_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:44:01.08 +18:08:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194169_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194169_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 194173_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194173_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:56:49.40 +24:12:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194185_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194185_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:06:04.13 +24:41:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194196_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194196_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 194199_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194199_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:33:18.18 +21:13:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194208_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194208_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:05:33.27 +24:17:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194216_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194216_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:06:14.67 +25:00:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.67, MAG_FAINT_SEARCH_LIMIT=15.65)GAIADR2_OUTPUT=# 1.553 3426551400108846592 091.56142522882 +25.00441824226 14.4460 13.5804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194217_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194217_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:55:41.33 +24:40:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194227_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
Preparing report for the candidate 194227_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
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Considering the candidate 194230_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194230_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:59:33.00 +26:51:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 2.488 3430037264286079360 089.88715852267 +26.86364818669 14.6876 13.9491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194238_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194238_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:59:03.95 +26:14:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 2.079 3429935563758235520 089.76590309691 +26.24293136092 14.6816 14.2318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194252_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194252_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 194262_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194262_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:57:33.28 +25:51:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 3.490 3429803343186352768 089.38953985074 +25.85431765043 14.6185 13.6461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194265_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194265_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 194266_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194266_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 194274_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194274_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 194276_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194276_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 194283_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194283_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 194291_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194291_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:03:24.31 +21:57:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.75, MAG_FAINT_SEARCH_LIMIT=15.73)GAIADR2_OUTPUT=# 1.299 3423634468775603968 090.85092087536 +21.96630745123 14.7583 14.1084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.299#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194307_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194307_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 194316_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194316_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:00:28.43 +26:20:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194319_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194319_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:05:31.24 +23:56:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194320_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194320_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 194329_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194329_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:46:29.77 +26:39:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194332_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194332_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:38:43.96 +17:15:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 2.220 3397414621147496832 084.68294360525 +17.25193993185 14.7111 14.1272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194350_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194350_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:05:36.61 +23:17:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 1.376 3423861552285943936 091.40247278135 +23.29887696932 14.6882 13.8843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194353_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194353_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:55:11.33 +25:17:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 1.860 3428280936196236544 088.79665160773 +25.29621671815 14.8948 14.2200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.860#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194366_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194366_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:05:21.83 +23:13:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 2.622 3423860792076281216 091.34023815679 +23.22155376451 14.6089 13.9184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194367_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194367_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 194371_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194371_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:01:23.87 +26:33:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 2.257 3429956866795719936 090.34905055341 +26.55509309304 14.5978 14.0352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194376_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194376_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:05:03.14 +26:12:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194377_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194377_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:59:48.94 +24:08:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194402_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194402_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 194403_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
Preparing report for the candidate 194403_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
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Considering the candidate 194404_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194404_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:34:31.85 +22:21:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194405_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194405_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:32:54.86 +22:25:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 1.172 3404033749865528448 083.22873439307 +22.42821060696 14.9344 14.2467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194411_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194411_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:42:00.61 +22:45:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 2.430 3403553709960389632 085.50190993925 +22.76553552732 15.1516 14.4900 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194433_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194433_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:55:57.41 +18:54:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 1.786 3398591094291801600 088.98907643338 +18.90998030422 14.8292 14.1534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194448_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194448_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 194475_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194475_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:35:44.60 +19:15:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 2.652 3400960992821907968 083.93506403548 +19.25173459556 14.9034 14.0878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194479_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194479_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:40:16.10 +19:35:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 1.769 3399480809653414528 085.06710274770 +19.59385219346 14.7604 14.1002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194489_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 194489_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 194529_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
Preparing report for the candidate 194529_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
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Considering the candidate 25845_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 25845_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 07287_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 07287_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:15:47.41 +26:45:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46902_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 46902_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 06:01:26.90 +23:51:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94871_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 94871_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 121964_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 121964_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 74248_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 74248_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:37:26.66 +22:20:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65501_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 65501_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 05101_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 05101_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:52:51.76 +26:47:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82933_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 82933_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:53:50.57 +21:45:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126539_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
Preparing report for the candidate 126539_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
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Considering the candidate 18235_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 18235_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 111854_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 111854_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
**** FOUND 05:55:48.83 +20:10:31.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 64676_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 64676_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 143024_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042
The candidate 143024_fd_Tau-04-Q1b1x1_2026-03-22_00-07-12_20.00sec_-14.90C_LIGHT_0042 did not pass the final checks