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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC
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 22.2125* 05 12 09.93 +20 36 21.4 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,2461121.7125,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2125 11.46CV 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-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:09.93 +20:36:21.4 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 46 02.66 +23 20 15.7 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,2461121.7125,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2125 11.51CV 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-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:02.66 +23:20:15.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 07 52.08 +18 13 12.3 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,2461121.7125,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2125 12.65CV 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-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:52.08 +18:13:12.3 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 09 53.70 +18 25 40.2 13.4 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
target,2461121.7125,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2125 13.39CV 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-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:09:53.70 +18:25:40.2 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 17 23.69 +19 07 24.1 13.7 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,2461121.7125,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2125 13.66CV 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-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:23.69 +19:07:24.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 33 43.67 +21 07 36.3 14.3 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,2461121.7125,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2125 14.32CV 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-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:33:43.67 +21:07:36.3 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 21 01.00 +23 44 23.8 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
NSVS J0521001+234443,2461121.7125,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0521001+234443 20260322.2125 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:21:01.00 +23:44:23.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 49 48.71 +25 25 23.0 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AY Tau,2461121.7125,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AY Tau 20260322.2125 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:48.71 +25:25:23.0 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 30 04.46 +25 01 43.2 13.3 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
NSVS 6923161,2461121.7125,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 6923161 20260322.2125 13.30CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:30:04.46 +25:01:43.2 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 18 56.76 +23 52 44.3 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
NSVS J0518565+235247,2461121.7125,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0518565+235247 20260322.2125 12.74CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:56.76 +23:52:44.3 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 33 29.18 +24 27 00.3 11.2 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
NSV 2118,2461121.7125,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 2118 20260322.2125 11.18CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:33:29.18 +24:27:00.3 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 46 18.01 +24 59 38.5 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
NSVS 6942167,2461121.7125,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 6942167 20260322.2125 12.74CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:18.01 +24:59:38.5 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 17 42.54 +21 41 23.0 12.2 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
NSVS J0517423+214125,2461121.7125,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0517423+214125 20260322.2125 12.24CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:42.54 +21:41:23.0 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 33 58.80 +26 06 49.7 13.2 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
ASASSN-V J053358.76+260651.1,2461121.7125,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053358.76+260651.1 20260322.2125 13.24CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:33:58.80 +26:06:49.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2125 2461121.7125 12.17 05:06:24.41 +19:19:14.2
183.12464 -12.75023 galactic Tau Second-epoch detections are separated by 0.6" and 4.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3407849295731372928 | 05:06:24.31 +19:19:16.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.886+/-0.026 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2125* 05 06 24.41 +19 19 14.2 12.2 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
Gaia DR3 3407849295731372928,2461121.7125,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3407849295731372928 20260322.2125 12.17CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:06:24.41 +19:19:14.2 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 16 29.04 +20 02 20.3 11.8 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
ASAS J051629+2002.4,2461121.7125,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J051629+2002.4 20260322.2125 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:16:29.04 +20:02:20.3 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 08 17.17 +21 56 44.0 11.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WX Tau,2461121.7125,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WX Tau 20260322.2125 11.93CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:08:17.17 +21:56:44.0 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 24 49.55 +23 06 05.6 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
NSV 1958,2461121.7125,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 1958 20260322.2125 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:24:49.55 +23:06:05.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 15 19.13 +23 53 43.0 12.4 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
NSVS 6906356,2461121.7125,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 6906356 20260322.2125 12.45CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:19.13 +23:53:43.0 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 13 57.21 +22 03 27.0 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
NSVS J0513571+220333,2461121.7125,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0513571+220333 20260322.2125 12.80CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:57.21 +22:03:27.0 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 06 48.24 +19 22 51.4 13.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J050647.96+192250.2,2461121.7125,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050647.96+192250.2 20260322.2125 12.97CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:06:48.24 +19:22:51.4 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 42 11.97 +24 53 06.2 13.5 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
Gaia DR3 3428806605832630144,2461121.7125,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3428806605832630144 20260322.2125 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:42:11.97 +24:53:06.2 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 22 21.62 +18 21 16.6 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,2461121.7125,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2125 12.74CV 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-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:22:21.62 +18:21:16.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2125 2461121.7125 13.43 06:01:15.51 +25:49:54.3
184.43673 1.41494 galactic Gem Second-epoch detections are separated by 1.2" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:01:15.51 +25:49:54.3 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7125,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2125 13.43CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:15.51 +25:49:54.3 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 28 44.56 +24 57 16.7 13.3 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
ASASSN-V J052844.51+245719.0,2461121.7125,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052844.51+245719.0 20260322.2125 13.32CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:28:44.56 +24:57:16.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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 22.2125* 05 32 32.99 +20 37 06.1 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
NSVS J0532328+203706,2461121.7125,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0532328+203706 20260322.2125 12.78CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:32:32.99 +20:37:06.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2125 2461121.7125 12.62 05:20:20.25 +18:58:49.4
185.30271 -10.22357 galactic Tau Second-epoch detections are separated by 0.4" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3401454020707738880 | 05:20:19.87 +18:58:48.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2125* 05 20 20.25 +18 58 49.4 12.6 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
Gaia DR3 3401454020707738880,2461121.7125,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3401454020707738880 20260322.2125 12.62CV 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:20:20.25 +18:58:49.4 ;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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20_00sec_-15_00C_LIGHT_0071_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20_00sec_-14_90C_LIGHT_0070_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Last image: 2461121.71281089 22.03.2026 05:06:16.861 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 38
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: 10 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): 19897
Objects passed selection criteria: 19884
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: 18974
Average stars matched: 18574.5 (97.8945 %)
Memory usage VmPeak: 124784 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 02:08:08 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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Last image: 2461121.71281089 22.03.2026 05:06:16.861 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 225
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
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: 76 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): 141006
Objects passed selection criteria: 140693
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 125006
Average stars matched: 121084 (96.8622 %)
Memory usage VmPeak: 2497156 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 02:11:14 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
SExtractor catalog cache: saved Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.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: 2461121.71226470
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits exists and is non-empty
Saving wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits to local_wcs_cache/
'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'local_wcs_cache/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits exists and is non-empty
Saving wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits to local_wcs_cache/
'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> 'local_wcs_cache/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits'
wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits'
wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.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 05:32:17.775 +21:59:26.78
Angular distance between the image centers 0.01 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 05:32:18.401 +21:59:03.44
Angular distance between the image centers 0.02 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 05:32:17.775 +21:59:26.78
Second-epoch second image center 05:32:18.401 +21:59:03.44
Angular distance between the image centers 0.00692 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits &> /tmp/tmp.wlYNh93QzK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits &> /tmp/tmp.AfIKjPfYlG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits &> /tmp/tmp.OjsbxPLfrH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits &> /tmp/tmp.rdKbOdwbSb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
Found non-empty wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
The reference image (wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits) and catalog (wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat) found
'wcs_Tau-04-Q2b1x1_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 27 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
2.0 pix Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
2.7 pix fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
2.7 pix fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
Limiting magnitude estimates:
15.3 mag. Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
15.3 mag. Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
14.9 mag. fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
14.9 mag. fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
All-image limiting magnitude estimate: 14.9 (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.wlYNh93QzK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'wcs_Tau-04-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -region wcs_Tau-04-Q2b1x1_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-Q2b1x1_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.AfIKjPfYlG (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> 'wcs_Tau-04-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits -region wcs_Tau-04-Q2b1x1_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-Q2b1x1_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.OjsbxPLfrH (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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1315, passed=19173
Got 19173 stars (including 17841 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits.cat
util/solve_plate_with_UCAC5 got 19173 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 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: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 933 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-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.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.rdKbOdwbSb (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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1254, passed=19054
Got 19054 stars (including 17782 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits.cat
util/solve_plate_with_UCAC5 got 19054 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
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 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.73"
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-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
Saving fully-calibrated image wcs_Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits'
Preparing the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31293.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out31278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31279.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 13s
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
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Considering the candidate 31273_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31273_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:49:09.60 +25:07:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.892 3428957646945087104 087.28998229715 +25.12158047831 12.2033 11.8741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31278_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 31278_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 31279_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 31279_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 31283_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31283_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:47:52.54 +23:25:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31284_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31284_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:47:46.37 +23:58:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31285_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31285_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:54:40.80 +24:40:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.982 3428037321354949888 088.66996982423 +24.67271573712 12.0959 11.5753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31291_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31291_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:30:53.99 +21:37:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31292_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31292_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:17:42.49 +21:41:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 1.244 3414593420881893888 079.42668205027 +21.68975417575 10.6311 9.2995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31293_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31293_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:35:22.00 +20:48:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.858 3402810848119383168 083.84175389792 +20.80072399780 11.9167 11.1159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31297_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31297_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:34:14.63 +23:02:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31299_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31299_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:31:11.79 +22:43:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31300_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31300_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:37:26.58 +22:20:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31301_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31301_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:44:16.82 +24:27:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31306_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31306_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:46:55.03 +22:19:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31307_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31307_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:35:40.73 +22:53:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 1.123 3404449326604738304 083.91970606065 +22.90020086262 12.2404 11.7443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.123#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31310_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31310_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:38:39.44 +22:33:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.939 3404201318013611648 084.66450148725 +22.56676496841 12.1719 11.6376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31313_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31313_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:53:43.40 +22:38:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 1.145 3424365094252484992 088.43099919159 +22.64919560495 12.1824 11.6406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31314_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31314_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:34:38.51 +22:32:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31315_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31315_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:36:10.12 +22:32:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31316_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31316_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:30:35.51 +23:55:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31317_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31317_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:39:57.34 +22:22:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.613 3403441040081814016 084.98884759737 +22.38201894028 12.2029 11.6421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31318_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31318_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:31:32.87 +21:03:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 1.472 3403616102947946368 082.88693876264 +21.05685289589 11.9876 11.1803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31319_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31319_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:35:44.74 +22:35:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 1.091 3404248528292221696 083.93656454006 +22.59504846260 12.1381 11.5965 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31323_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31323_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:59:15.34 +22:01:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.465 3424051458560844928 089.81416989804 +22.01788786452 12.1446 11.3876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31326_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31326_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:41:27.09 +20:46:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 3.600 3402667018256706688 085.36251405197 +20.78021898728 12.5583 12.1933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31330_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 31330_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:31:52.12 +17:53:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.020 3397394172806811776 082.96683203419 +17.89954516785 12.3873 11.8270 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14186_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 14186_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:55:48.71 +20:10:33.1 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 16s
Prepared the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:12:09.93 +20:36:21.4
05:46:02.66 +23:20:15.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
SExtractor catalog cache: saved Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Creating symlink local_wcs_cache/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits exists and is non-empty
wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.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 05:32:17.775 +21:59:26.78
Angular distance between the image centers 0.01 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 05:32:18.401 +21:59:03.44
Angular distance between the image centers 0.02 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 05:32:17.775 +21:59:26.78
Second-epoch second image center 05:32:18.401 +21:59:03.44
Angular distance between the image centers 0.00692 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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits &> /tmp/tmp.myn2P2xeu1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits &> /tmp/tmp.lTdB1FnuJe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits &> /tmp/tmp.bhjAmcFHLO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits &> /tmp/tmp.67xSdF2Znk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
Found non-empty wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
The reference image (wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits) and catalog (wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat) found
'wcs_Tau-04-Q2b1x1_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.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 108 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
1.9 pix Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
2.7 pix fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
2.8 pix fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
Limiting magnitude estimates:
15.5 mag. Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
15.5 mag. Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
14.9 mag. fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
14.9 mag. fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.2 (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.myn2P2xeu1 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'wcs_Tau-04-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -region wcs_Tau-04-Q2b1x1_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-Q2b1x1_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.lTdB1FnuJe (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> 'wcs_Tau-04-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits -region wcs_Tau-04-Q2b1x1_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-Q2b1x1_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.bhjAmcFHLO (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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=11745, passed=104640
Got 104640 stars (including 92776 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits.cat
util/solve_plate_with_UCAC5 got 104640 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
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: 0.60"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 931 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.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.67xSdF2Znk (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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=11383, passed=101595
Got 101595 stars (including 90111 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits.cat
util/solve_plate_with_UCAC5 got 101595 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
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: 0.61"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.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-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Saving fully-calibrated image wcs_Tau-04-Q2b1x1_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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-05-29_20.00sec_-14.90C_LIGHT_0070.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.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-Q2b1x1_020440_TTUQ2b1x1_4487_FcDcOLZC/wcs_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071.fits
Preparing the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out178568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out180999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out62537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out192544.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out104863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86534.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 25s
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: 12s
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Considering the candidate 192296_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192296_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:34:54.61 +17:43:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 3.314 3397687781066108288 083.72672360690 +17.71979549160 14.1674 13.0436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192316_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192316_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:39:28.97 +19:52:47.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)
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Considering the candidate 192318_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192318_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:38:22.77 +21:36:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 2.712 3403006737286022272 084.59480505406 +21.61522270392 14.2858 13.4349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192343_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192343_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 192351_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192351_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:23:51.34 +18:12:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.473 3400557197177136128 080.96357467220 +18.19977920995 13.6577 13.0340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192353_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192353_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:43:19.30 +25:42:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.903 3428920336567402496 085.83004887233 +25.70863399736 13.8448 13.2671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192360_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192360_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:19:24.14 +18:22:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 3.543 3395357190075971968 079.85112784510 +18.37483744370 13.9523 13.2950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192361_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192361_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:29:39.66 +25:57:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.318 3417867873885089408 082.41591877228 +25.95331349595 14.5207 13.7953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192372_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192372_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:52:15.34 +23:56:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192378_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192378_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:09:41.17 +18:14:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.278 3395526965839244416 077.42116796817 +18.24964590399 13.1379 12.3279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192379_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192379_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:20:41.78 +20:48:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 0.121 3414292292134568704 080.17410214372 +20.81030653922 13.2820 12.6613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192384_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192384_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:09:15.74 +17:54:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.429 3395136566196132352 077.31652071381 +17.91011188946 12.7340 11.9005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192386_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192386_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:48:21.31 +19:24:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192388_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192388_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:29:17.31 +18:20:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192400_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192400_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:46:02.72 +23:20:16.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192401_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192401_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:12:09.99 +20:36:22.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 192409_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192409_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:58:01.90 +25:55:16.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192433_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192433_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:20:11.85 +19:34:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192441_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 192441_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 192445_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192445_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:43:34.78 +25:27:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192451_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192451_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:51:30.90 +18:25:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 0.646 3398219291860293120 087.87861085439 +18.42431583682 12.6631 12.0467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192457_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192457_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:31:10.97 +20:10:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192475_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192475_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:48:27.21 +20:53:28.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192476_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192476_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:32:03.09 +18:33:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192487_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192487_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:58:09.53 +21:58:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192489_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192489_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:07:24.52 +18:37:09.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192490_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192490_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:55:14.62 +20:28:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192496_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192496_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:49:44.99 +24:06:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192508_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192508_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:47:05.73 +23:11:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 0.579 3427562160532776960 086.77398069312 +23.18718374888 12.8450 11.8024 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192515_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192515_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:15:08.81 +20:02:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 3.353 3413762537984956672 078.78572224152 +20.04054112115 13.0927 12.3216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192523_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192523_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:51:41.44 +23:14:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192531_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192531_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:41:06.98 +24:22:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.701 3428662913407508864 085.27935414376 +24.37095867275 13.4645 12.6986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192534_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192534_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:39:27.54 +21:47:29.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192540_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 192540_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 192541_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192541_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:17:30.51 +20:09:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 5.576 3413776792979249408 079.37650746996 +20.15651977221 13.4348 12.5808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192544_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192544_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:23:52.05 +20:00:17.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 192548_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192548_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:43:36.74 +25:27:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192555_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192555_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:49:12.05 +19:49:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.118 3399669852636525312 087.30029039364 +19.83058321241 13.5941 13.0857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192559_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192559_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:59:41.56 +19:52:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.810 3422766541785451264 089.92296759673 +19.88233881455 13.6037 13.0578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192561_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192561_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:36:40.75 +18:53:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192570_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192570_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:36:21.13 +24:22:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192572_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192572_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:19:43.98 +26:10:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192576_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192576_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:44:14.71 +21:13:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 2.558 3403072944204702592 086.06077309063 +21.21865959201 13.9715 13.0284 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192579_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192579_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:57:10.45 +21:28:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192580_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192580_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:53:58.55 +21:51:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192581_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192581_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:37:08.39 +22:06:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 0.775 3403787459261599232 084.28472618726 +22.10524376552 13.8073 13.2615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.775#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192582_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192582_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:58:05.55 +24:37:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192584_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192584_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:57:16.76 +22:22:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.695 3424134437328421760 089.32063409725 +22.37394336021 13.9322 13.3490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192585_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192585_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:34:57.16 +25:53:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192588_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192588_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:37:56.41 +22:27:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192597_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192597_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:49:58.17 +20:38:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192608_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 192608_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 192618_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192618_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:51:41.64 +22:53:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.769 3427387273760577792 087.92370106065 +22.89339370410 13.8936 13.4198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192620_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192620_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:24:43.22 +24:06:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192625_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192625_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:45:43.44 +20:40:02.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192629_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192629_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:47:37.28 +23:38:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192639_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192639_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:36:30.67 +25:57:47.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192643_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192643_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:50:26.44 +23:40:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192653_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192653_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:27:58.45 +21:26:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192666_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192666_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:31:04.88 +23:13:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 2.721 3416166276561542016 082.77030613945 +23.23136640704 14.2133 13.8115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192692_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192692_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 06:01:06.35 +21:01:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192695_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192695_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:47:39.88 +21:19:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 3.669 3400160612781356800 086.91706239529 +21.32214072232 14.4115 13.8329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192715_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192715_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:39:50.07 +19:23:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 4.930 3399453218783579648 084.95752341588 +19.39930871915 14.5647 14.0076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192724_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192724_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:41:48.15 +21:43:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192732_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192732_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:34:19.84 +20:16:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192736_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192736_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:39:28.78 +21:47:27.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192746_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192746_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:48:08.78 +21:07:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192754_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192754_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:46:04.88 +19:23:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192770_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 192770_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 192903_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192903_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 192955_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 192955_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 179944_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 179944_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
Rejecting candidate due to large distance (25.0") between the two second-epoch detections
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Considering the candidate 111854_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 111854_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:55:48.68 +20:10:33.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52744_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 52744_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 25835_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 25835_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 82933_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 82933_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:53:50.45 +21:45:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32970_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 32970_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 50562_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 50562_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 33017_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 33017_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:28:45.59 +25:02:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 4.816 3416958165451427584 082.19068825587 +25.04510728142 11.4454 10.4311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 42475_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 42475_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 190994_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 190994_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
Rejecting candidate due to large distance (25.5") between the two second-epoch detections
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Considering the candidate 32345_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 32345_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 86534_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 86534_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 16332_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 16332_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 21413_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 21413_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:33:39.68 +25:45:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.610 3441104604732343424 083.41644352315 +25.75504657259 13.5136 13.0078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 142509_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 142509_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 114972_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 114972_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 81205_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 81205_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 62999_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 62999_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 46902_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 46902_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 06:01:26.80 +23:51:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50295_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 50295_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 126932_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 126932_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
Rejecting candidate due to large distance (24.5") between the two second-epoch detections
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Considering the candidate 79591_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 79591_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 166509_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 166509_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:37:44.08 +17:45:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143437_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 143437_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 34402_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 34402_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
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Considering the candidate 74248_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 74248_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:37:26.62 +22:20:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62537_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 62537_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:59:15.18 +22:50:22.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
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Considering the candidate 77943_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 77943_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
Rejecting candidate due to large distance (24.4") between the two second-epoch detections
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Considering the candidate 180999_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 180999_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:10:20.96 +18:00:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 2.074 3395507685729256320 077.58675300110 +18.00263747920 13.6525 13.0581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126539_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 126539_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16566_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 16566_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34058_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 34058_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104863_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 104863_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136451_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
Preparing report for the candidate 136451_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179370_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 179370_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:22:16.66 +26:11:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 3.781 3418054687782404352 080.57016730486 +26.18508342442 10.5989 9.8280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179171_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 179171_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 06:01:38.87 +25:51:25.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
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Considering the candidate 178568_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071
The candidate 178568_fd_Tau-04-Q2b1x1_2026-03-22_00-06-16_20.00sec_-15.00C_LIGHT_0071 did not pass the final checks
**** FOUND 05:48:43.23 +18:04:00.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 42s
Prepared the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:12:09.93 +20:36:21.4
05:46:02.66 +23:20:15.7
05:32:32.99 +20:37:06.1
05:16:29.04 +20:02:20.3
05:22:21.62 +18:21:16.6
05:20:20.25 +18:58:49.4
05:06:24.41 +19:19:14.2
05:06:48.24 +19:22:51.4
05:33:58.80 +26:06:49.7
06:01:15.51 +25:49:54.3
05:07:52.08 +18:13:12.3
05:09:53.70 +18:25:40.2
05:17:23.69 +19:07:24.1
05:33:43.67 +21:07:36.3
05:49:48.71 +25:25:23.0
05:46:18.01 +24:59:38.5
05:30:04.46 +25:01:43.2
05:28:44.56 +24:57:16.7
05:42:11.97 +24:53:06.2
05:33:29.18 +24:27:00.3
05:15:19.13 +23:53:43.0
05:18:56.76 +23:52:44.3
05:21:01.00 +23:44:23.8
05:24:49.55 +23:06:05.6
05:13:57.21 +22:03:27.0
05:08:17.17 +21:56:44.0
05:17:42.54 +21:41:23.0
########### Completed Tau-04-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:12:09.93 +20:36:21.4
05:46:02.66 +23:20:15.7
05:07:52.08 +18:13:12.3
05:09:53.70 +18:25:40.2
05:17:23.69 +19:07:24.1
05:33:43.67 +21:07:36.3
05:21:01.00 +23:44:23.8
05:49:48.71 +25:25:23.0
05:30:04.46 +25:01:43.2
05:18:56.76 +23:52:44.3
05:33:29.18 +24:27:00.3
05:46:18.01 +24:59:38.5
05:17:42.54 +21:41:23.0
05:33:58.80 +26:06:49.7
05:06:24.41 +19:19:14.2
05:16:29.04 +20:02:20.3
05:08:17.17 +21:56:44.0
05:24:49.55 +23:06:05.6
05:15:19.13 +23:53:43.0
05:13:57.21 +22:03:27.0
05:06:48.24 +19:22:51.4
05:42:11.97 +24:53:06.2
05:22:21.62 +18:21:16.6
06:01:15.51 +25:49:54.3
05:28:44.56 +24:57:16.7
05:32:32.99 +20:37:06.1
05:20:20.25 +18:58:49.4
###################################################################################
05:12:09.93 +20:36:21.4 -- asteroid (will NOT add it to exclusion list)
05:46:02.66 +23:20:15.7 -- asteroid (will NOT add it to exclusion list)
05:07:52.08 +18:13:12.3 -- asteroid (will NOT add it to exclusion list)
05:09:53.70 +18:25:40.2 -- not an asteroid (will add it to exclusion list)
05:17:23.69 +19:07:24.1 -- asteroid (will NOT add it to exclusion list)
05:33:43.67 +21:07:36.3 -- asteroid (will NOT add it to exclusion list)
05:21:01.00 +23:44:23.8 -- not an asteroid (will add it to exclusion list)
05:49:48.71 +25:25:23.0 -- not an asteroid (will add it to exclusion list)
05:30:04.46 +25:01:43.2 -- not an asteroid (will add it to exclusion list)
05:18:56.76 +23:52:44.3 -- not an asteroid (will add it to exclusion list)
05:33:29.18 +24:27:00.3 -- not an asteroid (will add it to exclusion list)
05:46:18.01 +24:59:38.5 -- not an asteroid (will add it to exclusion list)
05:17:42.54 +21:41:23.0 -- not an asteroid (will add it to exclusion list)
05:33:58.80 +26:06:49.7 -- not an asteroid (will add it to exclusion list)
05:06:24.41 +19:19:14.2 -- not an asteroid (will add it to exclusion list)
05:16:29.04 +20:02:20.3 -- not an asteroid (will add it to exclusion list)
05:08:17.17 +21:56:44.0 -- not an asteroid (will add it to exclusion list)
05:24:49.55 +23:06:05.6 -- not an asteroid (will add it to exclusion list)
05:15:19.13 +23:53:43.0 -- not an asteroid (will add it to exclusion list)
05:13:57.21 +22:03:27.0 -- not an asteroid (will add it to exclusion list)
05:06:48.24 +19:22:51.4 -- not an asteroid (will add it to exclusion list)
05:42:11.97 +24:53:06.2 -- not an asteroid (will add it to exclusion list)
05:22:21.62 +18:21:16.6 -- asteroid (will NOT add it to exclusion list)
06:01:15.51 +25:49:54.3 -- not an asteroid (will add it to exclusion list)
05:28:44.56 +24:57:16.7 -- not an asteroid (will add it to exclusion list)
05:32:32.99 +20:37:06.1 -- not an asteroid (will add it to exclusion list)
05:20:20.25 +18:58:49.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:06:24.41 +19:19:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:48.24 +19:22:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:08:17.17 +21:56:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:09:53.70 +18:25:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:57.21 +22:03:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:19.13 +23:53:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:29.04 +20:02:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:42.54 +21:41:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:56.76 +23:52:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:20.25 +18:58:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:01.00 +23:44:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:49.55 +23:06:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:44.56 +24:57:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:04.46 +25:01:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:32.99 +20:37:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:29.18 +24:27:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:58.80 +26:06:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:11.97 +24:53:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:18.01 +24:59:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:48.71 +25:25:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:15.51 +25:49:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
05:06:24.41 +19:19:14.2 -- not a known variable star
05:06:48.24 +19:22:51.4 -- a known variable star
05:08:17.17 +21:56:44.0 -- a known variable star
05:09:53.70 +18:25:40.2 -- not a known variable star
05:13:57.21 +22:03:27.0 -- a known variable star
05:15:19.13 +23:53:43.0 -- a known variable star
05:16:29.04 +20:02:20.3 -- a known variable star
05:17:42.54 +21:41:23.0 -- a known variable star
05:18:56.76 +23:52:44.3 -- a known variable star
05:20:20.25 +18:58:49.4 -- not a known variable star
05:21:01.00 +23:44:23.8 -- a known variable star
05:24:49.55 +23:06:05.6 -- a known variable star
05:28:44.56 +24:57:16.7 -- a known variable star
05:30:04.46 +25:01:43.2 -- a known variable star
05:32:32.99 +20:37:06.1 -- a known variable star
05:33:29.18 +24:27:00.3 -- a known variable star
05:33:58.80 +26:06:49.7 -- a known variable star
05:42:11.97 +24:53:06.2 -- a known variable star
05:46:18.01 +24:59:38.5 -- a known variable star
05:49:48.71 +25:25:23.0 -- a known variable star
06:01:15.51 +25:49:54.3 -- not a known variable star
Found 4 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
21 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
Adding identified Gaia sources from exclusion_list_apass.txt
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
05:06:24.41 +19:19:14.2
05:06:48.24 +19:22:51.4
05:08:17.17 +21:56:44.0
05:09:53.70 +18:25:40.2
05:13:57.21 +22:03:27.0
05:15:19.13 +23:53:43.0
05:16:29.04 +20:02:20.3
05:17:42.54 +21:41:23.0
05:18:56.76 +23:52:44.3
05:20:20.25 +18:58:49.4
05:21:01.00 +23:44:23.8
05:24:49.55 +23:06:05.6
05:28:44.56 +24:57:16.7
05:30:04.46 +25:01:43.2
05:32:32.99 +20:37:06.1
05:33:29.18 +24:27:00.3
05:33:58.80 +26:06:49.7
05:42:11.97 +24:53:06.2
05:46:18.01 +24:59:38.5
05:49:48.71 +25:25:23.0
06:01:15.51 +25:49:54.3
05:49:09.60 +25:07:16.8
05:54:40.80 +24:40:20.8
05:17:42.49 +21:41:22.8
05:35:22.00 +20:48:01.8
05:35:40.73 +22:53:59.6
05:38:39.44 +22:33:59.6
05:53:43.40 +22:38:56.1
05:39:57.34 +22:22:54.7
05:31:32.87 +21:03:23.2
05:35:44.74 +22:35:41.2
05:59:15.34 +22:01:03.2
05:41:27.09 +20:46:45.4
05:31:52.12 +17:53:56.7
05:48:43.23 +18:04:00.6
06:01:38.87 +25:51:25.6
05:22:16.66 +26:11:03.4
05:10:20.96 +18:00:08.9
05:34:54.61 +17:43:09.5
05:39:28.97 +19:52:47.2
05:38:22.77 +21:36:52.1
05:23:51.34 +18:12:00.1
05:43:19.30 +25:42:29.6
05:19:24.14 +18:22:26.4
05:29:39.66 +25:57:11.1
05:09:41.17 +18:14:58.7
05:20:41.78 +20:48:37.0
05:09:15.74 +17:54:35.2
05:51:30.90 +18:25:27.1
05:47:05.73 +23:11:13.4
05:15:08.81 +20:02:25.6
05:41:06.98 +24:22:14.0
05:17:30.51 +20:09:18.3
05:49:12.05 +19:49:48.0
05:59:41.56 +19:52:58.1
05:44:14.71 +21:13:05.3
05:37:08.39 +22:06:18.9
05:57:16.76 +22:22:25.8
05:51:41.64 +22:53:36.6
05:31:04.88 +23:13:50.2
05:47:39.88 +21:19:17.6
05:39:50.07 +19:23:54.3
05:33:39.68 +25:45:17.9
05:28:45.59 +25:02:38.2
05:59:15.18 +22:50:22.6
05:23:52.05 +20:00:17.1
####################################################
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461121.71226470 -observatory 500
22:38:28.80 -07:53:06.2 Mercury (0.9mag)
01:12:05.85 +06:45:25.7 Venus (-3.9mag)
23:06:42.24 -06:52:05.6 Mars (1.2mag)
07:04:56.37 +22:57:47.8 Jupiter (-2.3mag)
00:17:54.24 -00:22:35.4 Saturn (0.9mag)
03:43:07.25 +19:32:29.8 Uranus (5.8mag)
00:07:27.52 -00:36:57.0 Neptune (7.8mag)
20:32:06.77 -22:53:38.1 Pluto (14.5mag)
02:36:55.82 +20:18:30.8 Moon (-9.1mag)
-rw-r--r-- 1 apache apache 361 Mar 22 02:08 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461121.71226470:
07:04:53.46 +22:57:55.9 Io (5.6mag)
07:05:01.17 +22:57:41.5 Europa (5.7mag)
07:04:39.84 +22:58:24.0 Ganymede (5.2mag)
07:04:18.45 +22:58:57.9 Callisto (6.4mag)
07:08:57.36 +22:58:42.2 Himalia (15.2mag)
07:04:52.13 +22:57:54.2 Thebe (16.1mag)
07:08:33.72 +23:22:30.9 Elara (17.2mag)
07:02:09.11 +23:50:50.2 Pasiphae (17.2mag)
07:13:42.82 +22:52:28.4 Carme (18.3mag)
00:17:52.88 -00:22:38.0 Titan (8.8mag)
00:17:58.33 -00:22:25.8 Rhea (10.1mag)
00:18:22.84 -00:20:29.4 Iapetus (11.5mag)
00:18:09.42 -00:22:36.1 Hyperion (14.8mag)
00:19:47.73 -00:11:25.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 22 02:08 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461121.71226470:
12:59:54.81 +07:33:31.9 JWST
18:19:09.72 +30:11:47.0 Chandra
16:46:59.66 -48:19:43.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 22 02:08 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461121.71226470 -observatory 500
-rw-r--r-- 1 apache apache 0 Mar 22 02:08 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
11:44:44.19 -62:10:45.50 ASASSN-26bq 2026-03-15.03 15.31
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 -0.22
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:25.13 +04:00:01.40 SN 2026kc 2026-01-18.24 16.4
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
-rw-r--r-- 1 apache apache 5.7K Mar 22 02:08 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 22 02:08 tocp_transients_list.txt