This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.1536* 09 34 59.19 +07 59 19.0 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.6536,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.1536 12.73CV 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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:34:59.19 +07:59:19.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_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
GZ Cnc,2461125.6536,13.86,0.05,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
GZ Cnc 20260326.1536 13.86CV 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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:15:51.51 +09:00:49.9 ;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-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.6536,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.1536 13.89CV 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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:35:35.37 +03:34:35.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.6536,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.1536 14.38CV 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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:52.84 +08:46:26.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.1536* 09 36 07.87 +08 11 30.7 14.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.6536,14.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.1536 14.49CV 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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:36:07.87 +08:11:30.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.6536,14.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.1536 14.59CV 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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:59:13.03 +05:36:21.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.1536* 09 42 43.89 +05 24 38.4 14.6 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
VARIABLE_NAME,2461125.6536,14.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.1536 14.58CV 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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:42:43.89 +05:24:38.4 ;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-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.1536* 09 48 15.70 +09 05 41.8 13.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.6536,13.38,0.05,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 20260326.1536 13.38CV 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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:48:15.70 +09:05:41.8 ;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-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20_00sec_-10_00C_LIGHT_0351_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20_00sec_-15_00C_LIGHT_0191_fits__*pix.png resample_wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20_00sec_-10_00C_LIGHT_0350_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: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
First image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Last image: 2461125.65389083 26.03.2026 03:41:26.168 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8092
Objects passed selection criteria: 8080
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 7226.25
Average stars matched: 7052.5 (97.5956 %)
Memory usage VmPeak: 114364 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 22:47:18 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: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
First image: 2461093.74633115 22.02.2026 05:54:33.011 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Last image: 2461125.65389083 26.03.2026 03:41:26.168 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 107
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 13 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): 45561
Objects passed selection criteria: 45455
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 41462
Average stars matched: 40202.5 (96.9623 %)
Memory usage VmPeak: 147348 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 22:48:01 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.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: 2461125.65336823
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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits exists and is non-empty
Saving wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits to local_wcs_cache/
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits exists and is non-empty
Saving wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits to local_wcs_cache/
'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits'
wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:25.146 +06:02:19.62
Angular distance between the image centers 0.08 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 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:23.629 +06:02:15.98
Angular distance between the image centers 0.09 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 09:25:25.146 +06:02:19.62
Second-epoch second image center 09:25:23.629 +06:02:15.98
Angular distance between the image centers 0.00637 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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits &> /tmp/tmp.BVCiHL1dAM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits &> /tmp/tmp.fAWWGF7I2U
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits &> /tmp/tmp.UP2i3Nnt20
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits &> /tmp/tmp.UFKN48XP1d
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
The reference image (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits) and catalog (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat) found
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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 5047 out of 9705 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.925124
a=0.000000 b=1.000000 c=22.925124
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
2.5 pix Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
2.5 pix fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
2.5 pix fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
Limiting magnitude estimates:
15.3 mag. Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
15.3 mag. Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
14.8 mag. fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
14.9 mag. fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
All-image limiting magnitude estimate: 14.8 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.BVCiHL1dAM (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=629, passed=9705
Got 9705 stars (including 9071 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
util/solve_plate_with_UCAC5 got 9705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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.fAWWGF7I2U (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=616, passed=9704
Got 9704 stars (including 9075 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
util/solve_plate_with_UCAC5 got 9704 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 940 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
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 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 937 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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.UP2i3Nnt20 (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_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.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_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=428, passed=7219
Got 7219 stars (including 6788 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits.cat
util/solve_plate_with_UCAC5 got 7219 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits -region wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.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.UFKN48XP1d (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_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.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_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=449, passed=7205
Got 7205 stars (including 6748 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits.cat
util/solve_plate_with_UCAC5 got 7205 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 937 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits -region wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits'
Preparing the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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 20483_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 20483_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:41:13.72 +09:54:36.7 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Creating symlink local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits exists and is non-empty
wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:25.146 +06:02:19.62
Angular distance between the image centers 0.08 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 09:25:43.014 +06:00:02.92
Second-epoch image center 09:25:23.629 +06:02:15.98
Angular distance between the image centers 0.09 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 09:25:25.146 +06:02:19.62
Second-epoch second image center 09:25:23.629 +06:02:15.98
Angular distance between the image centers 0.00637 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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits &> /tmp/tmp.wiSN3Ndq4H
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits &> /tmp/tmp.8ltUXxzmoa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits &> /tmp/tmp.cYAkj01iYp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits &> /tmp/tmp.11z1p9qN5S
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
Found non-empty wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits and wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
The reference image (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits) and catalog (wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat) found
'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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 5088 out of 52265 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.799339
a=0.000000 b=1.000000 c=22.799339
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 79 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
2.3 pix Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
2.4 pix fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
2.3 pix fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
Limiting magnitude estimates:
15.4 mag. Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
15.4 mag. Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
15.0 mag. fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
15.0 mag. fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.wiSN3Ndq4H (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=3222, passed=52238
Got 52238 stars (including 48939 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat
util/solve_plate_with_UCAC5 got 52238 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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.8ltUXxzmoa (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits' -> 'wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat corresponding to the image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=3213, passed=52136
Got 52136 stars (including 48850 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat
util/solve_plate_with_UCAC5 got 52136 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits -region wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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.cYAkj01iYp (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_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.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_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1915, passed=39473
Got 39473 stars (including 37517 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits.cat
util/solve_plate_with_UCAC5 got 39473 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits -region wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.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.11z1p9qN5S (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_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.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_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits.cat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=2034, passed=40019
Got 40019 stars (including 37936 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits.cat
util/solve_plate_with_UCAC5 got 40019 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 937 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: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits -region wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.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-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.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_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/wcs_Hya-02-Q2b1x1_2026-02-21_23-54-33_20.00sec_-15.00C_LIGHT_0191.fits
Saving fully-calibrated image wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.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_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/wcs_Hya-02-Q2b1x1_2026-02-21_23-55-20_20.00sec_-14.90C_LIGHT_0192.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.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_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-40-41_20.00sec_-10.00C_LIGHT_0350.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.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_2026-03-25_CI_Hya-02-Q2b1x1_224510_TTUQ2b1x1_707_wn0i45qT/wcs_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351.fits
Preparing the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out65572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out66426.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out41393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66820.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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: 4s
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Considering the candidate 65572_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 65572_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:29:01.72 +04:10:46.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)
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Considering the candidate 65574_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 65574_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:19:30.66 +09:53:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.731 590801240083579136 139.87823646081 +09.88937595722 14.2616 13.7387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65579_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 65579_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:14:25.09 +07:54:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 1.308 590114904309970944 138.60490824349 +07.90439933873 13.8387 13.3404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65582_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 65582_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:06:37.39 +02:50:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65584_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 65584_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:32:28.23 +09:05:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 1.317 588239755947694336 143.11777555371 +09.09030452749 11.7508 11.2724 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65647_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 65647_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:41:13.72 +09:54:36.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 65760_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 65760_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 65876_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 65876_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 65887_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 65887_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:10:35.89 +07:33:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 3.328 589996668154899456 137.64981974187 +07.56693804964 12.5592 11.8798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65919_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
Preparing report for the candidate 65919_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
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Considering the candidate 65920_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 65920_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:04:12.98 +06:41:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65927_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 65927_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:09:02.52 +07:29:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65968_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 65968_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:37:19.01 +06:51:32.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 66041_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66041_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 66158_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66158_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:14:28.58 +07:47:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66182_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66182_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:09:49.98 +10:12:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66200_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66200_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:37:17.51 +06:48:25.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 66256_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66256_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 66306_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66306_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 66321_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66321_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:23:44.48 +05:14:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66342_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
Preparing report for the candidate 66342_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
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Considering the candidate 66350_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66350_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 66399_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66399_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 66413_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66413_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:32:45.16 +01:52:58.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 66426_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66426_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:32:14.18 +08:54:57.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)
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Considering the candidate 66427_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66427_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:14:28.89 +02:20:15.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 66443_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66443_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 66469_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66469_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:13:32.58 +02:56:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 2.796 578757602030092160 138.38580008418 +02.93724727558 14.1902 13.6711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66482_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66482_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:46:56.44 +07:05:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 3.784 3853754273573862528 146.73410925834 +07.08868710430 14.2812 13.7257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.784#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66487_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
Preparing report for the candidate 66487_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
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Considering the candidate 66491_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66491_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 66507_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66507_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:29:41.68 +09:54:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 2.496 589115448239842432 142.42379203880 +09.90640114205 14.2728 13.7960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66514_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66514_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 66548_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66548_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:21:19.64 +05:31:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66554_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66554_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:14:28.07 +08:28:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.978 590220079469022464 138.61747863355 +08.47680753940 14.2886 13.7743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66555_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66555_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:23:35.63 +06:23:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 2.258 585929956895719808 140.89906784353 +06.38669015329 14.2431 13.7812 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66565_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66565_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:24:20.57 +04:45:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.870 3852069070141159680 141.08518938759 +04.76049264503 14.4611 13.7857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66567_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66567_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 66582_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66582_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 66593_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66593_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:11:55.88 +09:43:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 2.856 590912703074675072 137.98353889331 +09.73100711217 14.1400 13.5732 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66594_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66594_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 66596_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66596_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:38:26.72 +07:42:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 3.914 3854458171469608064 144.61241552673 +07.70501495924 14.3275 13.8734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66603_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66603_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:15:54.08 +08:13:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66605_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66605_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 66606_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
Preparing report for the candidate 66606_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
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Considering the candidate 66610_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66610_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:19:43.36 +10:03:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.303 590813811452838016 139.93085614606 +10.06346774049 14.3226 13.5340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66650_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66650_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:10:06.40 +08:56:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 3.055 590477605707806976 137.52740781887 +08.93884546892 14.7342 14.1121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66652_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66652_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 66654_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66654_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 66660_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66660_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 66694_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66694_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 66704_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66704_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 66709_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66709_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 66712_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66712_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 66771_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
Preparing report for the candidate 66771_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
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Considering the candidate 66780_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
Preparing report for the candidate 66780_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
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Considering the candidate 66781_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66781_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 66786_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66786_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 08:59:47.19 +09:12:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 2.428 585440777300609152 134.94729461938 +09.21097673426 14.5854 14.0516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66787_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66787_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 66790_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66790_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 66799_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66799_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 66804_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66804_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 66807_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66807_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 66817_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66817_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 08:57:58.62 +06:33:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 0.533 583729902848341888 134.49422529574 +06.56582608811 15.0496 14.3510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66820_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
Preparing report for the candidate 66820_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
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Considering the candidate 66821_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66821_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 66822_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66822_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:04:59.97 +09:37:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 2.502 591429645338353408 136.25056218587 +09.62248412566 14.9200 14.4396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66825_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66825_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 66835_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66835_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 66840_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66840_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 66861_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66861_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 66865_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66865_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 66881_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66881_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 66883_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66883_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 66893_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66893_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
**** FOUND 09:09:48.44 +08:48:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 0.679 590466198274677760 137.45202395298 +08.81074206530 14.9634 14.4766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66901_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66901_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 66927_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 66927_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 41393_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
Preparing report for the candidate 41393_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
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Considering the candidate 63746_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351
The candidate 63746_fd_Hya-02-Q2b1x1_2026-03-25_22-41-26_20.00sec_-10.00C_LIGHT_0351 did not pass the final checks