This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
X Hya,2461118.8089,8.64,0.05,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
X Hya 20260319.3089 8.64CV 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/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:35:30.02 -14:41:25.2 ;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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8089,13.95,0.05,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 20260319.3089 13.95CV 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/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:57:32.50 -04:50:29.5 ;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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5733764714343010176,2461118.8089,13.64,0.05,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 5733764714343010176 20260319.3089 13.64CV 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/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:55:01.68 -14:47:38.8 ;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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8089,13.76,0.05,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 20260319.3089 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:57:23.62 -05:45:26.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8089,13.46,0.05,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
target 20260319.3089 13.46CV 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/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:59:12.31 -04:49:55.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3089 2461118.8089 13.29 08:56:19.66 -05:17:23.8
233.37529 24.66621 galactic Hya Second-epoch detections are separated by 4.1" and 8.9 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 5760718997083401088 | 08:56:20.24 -05:17:26.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (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
Gaia DR3 5760718997083401088,2461118.8089,13.29,0.05,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 5760718997083401088 20260319.3089 13.29CV 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/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:56:19.66 -05:17:23.8 ;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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3089 2461118.8089 12.87 08:55:32.59 -06:03:13.3
233.95921 24.08439 galactic Hya Second-epoch detections are separated by 1.2" and 8.7 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 5757649027475822464 | 08:55:33.18 -06:03:15.5 (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!
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 5757649027475822464,2461118.8089,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5757649027475822464 20260319.3089 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:55:32.59 -06:03:13.3 ;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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5757694176171932032,2461118.8089,12.11,0.05,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 5757694176171932032 20260319.3089 12.11CV 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/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:56:23.32 -05:47:10.8 ;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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3089 2461118.8089 14.13 09:52:41.81 -09:39:06.3
247.00075 33.18590 galactic Sex Second-epoch detections are separated by 6.1" and 9.2 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 3770860412624078080 | 09:52:41.28 -09:38:36.1 (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 19.3089* 09 52 41.81 -09 39 06.3 14.1 U Sex 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 3770860412624078080,2461118.8089,14.13,0.05,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 3770860412624078080 20260319.3089 14.13CV 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/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:52:41.81 -09:39:06.3 ;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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DI Hya,2461118.8089,11.88,0.05,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
DI Hya 20260319.3089 11.88CV 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/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:51.26 -12:31:36.4 ;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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20_00sec_-14_90C_LIGHT_0020_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20_00sec_-15_00C_LIGHT_0474_fits__*pix.png resample_wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20_00sec_-14_90C_LIGHT_0019_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: 2461032.88320810 23.12.2025 09:11:39.180 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
First image: 2461032.88320810 23.12.2025 09:11:39.180 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
Last image: 2461118.80922351 19.03.2026 07:25:06.911 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.82
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: 5 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): 11236
Objects passed selection criteria: 11232
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: 10686.5
Average stars matched: 10445 (97.7401 %)
Memory usage VmPeak: 116428 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 02:35:56 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: 2461032.88320810 23.12.2025 09:11:39.180 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
First image: 2461032.88320810 23.12.2025 09:11:39.180 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
Last image: 2461118.80922351 19.03.2026 07:25:06.911 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 165
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
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: 27 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): 67433
Objects passed selection criteria: 67309
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 62885.8
Average stars matched: 60634 (96.4193 %)
Memory usage VmPeak: 1988180 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 02:37:30 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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
SExtractor catalog cache: saved Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat to cache
SExtractor catalog cache: saved Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.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/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.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: 2461118.80863513
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits exists and is non-empty
Saving wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits to local_wcs_cache/
'wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits' -> 'local_wcs_cache/wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits'
wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits exists and is non-empty
Saving wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits to local_wcs_cache/
'wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits' -> 'local_wcs_cache/wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits'
wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits exists and is non-empty
Saving wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits to local_wcs_cache/
'wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits'
wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits exists and is non-empty
Saving wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits to local_wcs_cache/
'wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits' -> 'local_wcs_cache/wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.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 09:25:56.068 -09:59:34.09
Second-epoch image center 09:25:38.655 -10:03:14.83
Angular distance between the image centers 0.09 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:56.068 -09:59:34.09
Second-epoch image center 09:25:41.594 -10:02:47.66
Angular distance between the image centers 0.08 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 09:25:38.655 -10:03:14.83
Second-epoch second image center 09:25:41.594 -10:02:47.66
Angular distance between the image centers 0.01422 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/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits &> /tmp/tmp.lvvweyso3N
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits &> /tmp/tmp.nbftX4Glvf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits &> /tmp/tmp.1gVNs8lvli
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits &> /tmp/tmp.cd4K4k3X1f
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits and wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits and wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat
Found non-empty wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits and wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat
The reference image (wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits) and catalog (wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat) found
'wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.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 6729 out of 11198 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.924644
a=0.000000 b=1.000000 c=22.924644
From vast_summary.log: estimated ref. image limiting mag.: -7.82
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.10
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.10
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
2.1 pix Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
2.4 pix fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
2.4 pix fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
Limiting magnitude estimates:
15.1 mag. Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
15.1 mag. Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
14.9 mag. fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
14.9 mag. fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.lvvweyso3N (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/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits' -> 'wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
WCS_IMAGE_NAME=wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
WCS-calibrated image found: wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
Checking if the catalog wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat corresponding to the image wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits alredy exist and is non-empty...
Catalog wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat corresponding to the image wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
WCS catalog name: wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=759, passed=11198
Got 11198 stars (including 10418 good ones) from the SExtractor catalog wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat
util/solve_plate_with_UCAC5 got 11198 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 949 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: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
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 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.26"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits -region wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.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.nbftX4Glvf (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/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits' -> 'wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
WCS_IMAGE_NAME=wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
WCS-calibrated image found: wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
Checking if the catalog wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat corresponding to the image wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits alredy exist and is non-empty...
Catalog wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat corresponding to the image wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
WCS catalog name: wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=779, passed=11235
Got 11235 stars (including 10439 good ones) from the SExtractor catalog wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat
util/solve_plate_with_UCAC5 got 11235 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 949 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: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
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 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits -region wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.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.1gVNs8lvli (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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
Checking if the catalog wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
WCS catalog name: wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=584, passed=10320
Got 10320 stars (including 9726 good ones) from the SExtractor catalog wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 10320 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 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: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits -region wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.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.cd4K4k3X1f (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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
WCS-calibrated image found: wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
Checking if the catalog wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
WCS catalog name: wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=570, passed=10277
Got 10277 stars (including 9700 good ones) from the SExtractor catalog wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 10277 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 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: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits -region wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits'
Saving fully-calibrated image wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits'
Saving fully-calibrated image wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits'
Saving fully-calibrated image wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits'
Preparing the HTML report for the field Hya-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20669.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out00613.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20589_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 20589_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:49:05.59 -06:17:39.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20598_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 20598_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:11:14.59 -09:22:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20602_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 20602_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:24:50.35 -06:47:34.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20669_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 20669_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:06:51.26 -12:31:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 1.025 5735960262968825472 136.71385671726 -12.52687695070 12.1034 11.8310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20692_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 20692_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:24:24.88 -10:13:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.565 5739745988878184448 141.10370820179 -10.21798478183 12.1109 11.7581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00613_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
Preparing report for the candidate 00613_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Hya-06-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 ####
09:35:30.02 -14:41:25.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
SExtractor catalog cache: saved Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat to cache
SExtractor catalog cache: saved Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
Creating symlink local_wcs_cache/wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits exists and is non-empty
wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits exists and is non-empty
wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits exists and is non-empty
wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.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 09:25:56.068 -09:59:34.09
Second-epoch image center 09:25:38.655 -10:03:14.83
Angular distance between the image centers 0.09 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:56.068 -09:59:34.09
Second-epoch image center 09:25:41.594 -10:02:47.66
Angular distance between the image centers 0.08 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 09:25:38.655 -10:03:14.83
Second-epoch second image center 09:25:41.594 -10:02:47.66
Angular distance between the image centers 0.01422 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/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits &> /tmp/tmp.LK7EssA8xa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits &> /tmp/tmp.aubqvjxHG9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits &> /tmp/tmp.qIK9VFqu1z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits &> /tmp/tmp.sfveBzxdrs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits and wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits and wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat
Found non-empty wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits and wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat
The reference image (wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits) and catalog (wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat) found
'wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.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 6936 out of 68994 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.807069
a=0.000000 b=1.000000 c=22.807069
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.24
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.24
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 68 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
2.0 pix Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
2.3 pix fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
2.3 pix fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
Limiting magnitude estimates:
15.2 mag. Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
15.2 mag. Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
15.0 mag. fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
15.0 mag. fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.LK7EssA8xa (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/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits' -> 'wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
WCS_IMAGE_NAME=wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
WCS-calibrated image found: wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
Checking if the catalog wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat corresponding to the image wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits alredy exist and is non-empty...
Catalog wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat corresponding to the image wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
WCS catalog name: wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=3761, passed=68987
Got 68987 stars (including 65097 good ones) from the SExtractor catalog wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat
util/solve_plate_with_UCAC5 got 68987 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 946 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: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits -region wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.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.aubqvjxHG9 (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/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits' -> 'wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
WCS_IMAGE_NAME=wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
WCS-calibrated image found: wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
Checking if the catalog wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat corresponding to the image wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits alredy exist and is non-empty...
Catalog wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat corresponding to the image wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
WCS catalog name: wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=3796, passed=69456
Got 69456 stars (including 65526 good ones) from the SExtractor catalog wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat
util/solve_plate_with_UCAC5 got 69456 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 945 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: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits -region wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.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.qIK9VFqu1z (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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
Checking if the catalog wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
WCS catalog name: wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=3157, passed=57458
Got 57458 stars (including 54237 good ones) from the SExtractor catalog wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 57458 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
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: 0.52"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits -region wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.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.sfveBzxdrs (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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
WCS-calibrated image found: wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
Checking if the catalog wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
WCS catalog name: wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=3145, passed=57362
Got 57362 stars (including 54146 good ones) from the SExtractor catalog wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 57362 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits -region wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.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_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/wcs_Hya-06-Q2b1x1_2025-12-23_03-11-39_20.00sec_-15.00C_LIGHT_0474.fits
Saving fully-calibrated image wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/wcs_Hya-06-Q2b1x1_2025-12-23_03-12-16_20.00sec_-15.00C_LIGHT_0475.fits
Saving fully-calibrated image wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-24-16_20.00sec_-14.90C_LIGHT_0019.fits
Saving fully-calibrated image wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.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_2026-03-19_CI_Hya-06-Q2b1x1_023157_TTUQ2b1x1_7216_pcWLioBS/wcs_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020.fits
Preparing the HTML report for the field Hya-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out84417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out84878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85141.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85176.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out18375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84467.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85173.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 23s
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: 6s
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Considering the candidate 84417_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84417_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:40:35.41 -14:27:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.031 5688841246211967104 145.14736745766 -14.45175909380 14.3223 13.7553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84420_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84420_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:50:41.42 -08:03:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.963 3819641963977353216 147.67240386705 -08.05928334936 14.2760 13.7958 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84422_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84422_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:53:35.09 -06:13:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 0.791 3821612769850567168 148.39618959748 -06.22430220470 14.3001 13.7531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84423_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84423_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:33:46.44 -13:43:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84428_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84428_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:50:11.21 -14:55:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.079 5687031724950649600 147.54642470856 -14.92523948410 14.2760 13.7611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84440_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84440_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:41:21.43 -11:58:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.313 5691650876377934336 145.33951833835 -11.97937289015 13.8654 13.3189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84447_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84447_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:45:04.06 -12:20:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 2.057 5690834592073502208 146.26715182932 -12.34957878565 13.7958 13.1780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84449_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84449_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:05:46.81 -10:07:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.805 5743321836914513536 136.44553907508 -10.12246921657 14.0842 13.6134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84462_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84462_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 08:57:55.24 -05:57:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 3.453 5757630129619665024 134.48107620527 -05.95281860093 13.1065 12.4606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84463_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84463_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:47:12.39 -14:23:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84465_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
Preparing report for the candidate 84465_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
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Considering the candidate 84467_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
Preparing report for the candidate 84467_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
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Considering the candidate 84476_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84476_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:52:05.58 -10:40:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84480_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
Preparing report for the candidate 84480_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
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Considering the candidate 84481_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84481_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 08:54:28.89 -14:38:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.101 5733780794700569344 133.62119742141 -14.64569106332 13.0078 12.4159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84482_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84482_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:25:26.28 -06:50:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.220 5745317867131026688 141.35942557018 -06.84730667167 13.6285 13.1221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84487_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84487_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:47:26.39 -10:04:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.764 3770924974572604032 146.86014429750 -10.08287129389 13.6458 13.0143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84488_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84488_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 08:57:39.93 -05:57:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 3.584 5757628858309351808 134.41730168170 -05.95323751356 12.7752 12.1527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84490_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84490_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 08:55:08.42 -13:53:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.447 5734122158701365120 133.78573298814 -13.89083714861 12.9277 12.2704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84496_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84496_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 08:55:34.56 -06:28:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 4.016 5757211623710335616 133.89488731797 -06.47885011948 12.8410 12.4110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84501_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
Preparing report for the candidate 84501_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
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Considering the candidate 84503_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84503_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 08:57:41.43 -05:23:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 4.461 5757804397916586112 134.42376807356 -05.38785141322 12.8342 12.3142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84505_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
Preparing report for the candidate 84505_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
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Considering the candidate 84511_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84511_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:48:20.58 -06:15:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84512_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84512_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 08:54:25.37 -13:55:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 2.304 5734101405419415040 133.60633607411 -13.93036235717 12.8142 12.3393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.304#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84515_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84515_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 08:56:15.94 -04:50:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.112 5760888188731208704 134.06718488390 -04.85001277631 12.6076 11.9300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84531_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84531_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:15:34.72 -07:58:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 0.527 5745539384364424960 138.89471081846 -07.97844523375 13.3127 12.8696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84536_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84536_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 08:54:23.58 -14:24:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.298 5734067934739182592 133.59858497424 -14.41634288112 12.3715 11.7205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84541_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84541_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:54:22.34 -13:56:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84546_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
Preparing report for the candidate 84546_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
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Considering the candidate 84549_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84549_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:55:32.25 -14:27:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.266 5687111813204820864 148.88498174787 -14.45678124120 12.6130 11.8286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84553_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84553_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:51:04.50 -13:19:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.984 5687854194008096128 147.76900806481 -13.32938589574 12.2486 11.5422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84554_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84554_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:46:29.03 -05:15:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84556_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
Preparing report for the candidate 84556_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
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Considering the candidate 84650_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84650_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:11:42.29 -12:09:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 2.313 5733077515279277568 137.92685936262 -12.15338468217 12.4294 11.7650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84705_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84705_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:35:52.68 -05:22:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84878_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84878_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:42:08.12 -15:08:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.334 5685653555844697216 145.53378709210 -15.13923000115 13.4812 12.6633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.334#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 84893_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84893_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:19:29.82 -11:17:47.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 84914_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 84914_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:43:03.86 -13:14:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85016_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85016_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:33:47.87 -14:43:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85091_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85091_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:08:21.65 -06:10:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 3.702 5758161709131786112 137.09014021699 -06.18347047884 14.0740 13.5922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85123_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85123_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:15:17.38 -08:28:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 2.461 5743962100574885376 138.82174736497 -08.47230177530 14.0026 13.5973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85128_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85128_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:09:36.12 -09:56:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 2.894 5742616676299433472 137.40018709758 -09.95032577798 14.0349 13.5861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85132_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85132_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:52:58.80 -11:32:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.753 5691140080212579968 148.24494881613 -11.53720650143 14.2861 13.3525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85141_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85141_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:49:00.29 -14:10:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 4.279 5687319315960806528 147.25240420123 -14.16889982422 14.4510 13.9438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85162_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85162_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:32:49.00 -09:08:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.404 5741600006000608768 143.20390164006 -09.13837255630 14.3783 13.8103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85173_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
Preparing report for the candidate 85173_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
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Considering the candidate 85176_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85176_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:52:11.01 -09:28:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 2.578 3770879585358085504 148.04660065548 -09.47144624780 14.3443 13.7167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.578#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85191_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85191_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:56:51.57 -05:36:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.722 3821743130697992704 149.21470230315 -05.61059123951 14.3552 13.8860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85194_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85194_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:56:10.08 -08:12:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 1.672 3771630826677914624 149.04199169537 -08.21424221114 14.3592 13.8980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85206_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85206_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:28:25.46 -06:44:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 3.075 5745356315678342144 142.10541341391 -06.73714668850 14.4966 13.5343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85225_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85225_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:31:43.31 -10:34:13.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 85233_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85233_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:49:39.62 -05:13:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 1.888 3822530071785728128 147.41473280280 -05.21880802259 14.3635 13.7981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85248_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85248_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:44:48.65 -07:17:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.526 3819614338747759872 146.20308807173 -07.28761102987 14.2844 13.5365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85253_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85253_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:53:54.05 -10:11:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 2.422 3770028391559502976 148.47539078990 -10.18748166276 14.4514 13.9042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85257_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85257_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:33:59.73 -06:22:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 1.899 3823668822234830976 143.49884743920 -06.37649904153 14.3789 13.7651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85270_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85270_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:45:03.77 -14:40:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 1.346 5685787593183985024 146.26597907041 -14.67110000393 14.3547 13.7368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85274_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85274_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:53:04.49 -12:39:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 0.403 5690907743956744448 148.26870960939 -12.65483411101 14.5065 13.8690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85286_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85286_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:48:49.46 -05:31:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 2.344 3822506226127314176 147.20626787930 -05.52070786459 14.6744 14.2412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85326_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85326_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:23:37.04 -12:48:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 4.189 5738047964967815680 140.90336367450 -12.81437269164 14.7529 14.2812 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85334_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85334_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:54:48.46 -08:02:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.570 3771694731496173696 148.70263716576 -08.03755798654 14.5315 14.0581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85349_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85349_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:44:39.75 -06:05:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.401 3820879425658963328 146.16601657430 -06.10001357217 14.5654 14.0017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85396_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85396_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 85459_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 85459_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:53:43.70 -09:31:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 1.913 3770885770111048064 148.43233394988 -09.52858150018 14.6141 14.1744 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 40724_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 40724_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:11:14.59 -09:22:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03099_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 03099_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks
**** FOUND 09:35:30.03 -14:41:25.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 18375_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
Preparing report for the candidate 18375_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
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Considering the candidate 57315_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020
The candidate 57315_fd_Hya-06-Q2b1x1_2026-03-19_02-25-06_20.00sec_-14.90C_LIGHT_0020 did not pass the final checks