This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461082.7586,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260211.2586 12.28CV 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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:00:07.99 +02:03:56.8 ;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-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20_00sec_-15_00C_LIGHT_0238_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20_00sec_-15_00C_LIGHT_0237_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-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20_00sec_-15_00C_LIGHT_0238_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20_00sec_-15_00C_LIGHT_0237_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,2461082.7586,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GZ Cnc 20260211.2586 13.31CV 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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:15:51.50 +09:00:49.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20_00sec_-15_00C_LIGHT_0238_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20_00sec_-15_00C_LIGHT_0237_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-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20_00sec_-15_00C_LIGHT_0238_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20_00sec_-15_00C_LIGHT_0237_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 02 11.2585* 09 50 01.98 +08 25 23.6 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
VARIABLE_NAME,2461082.7586,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260211.2586 13.44CV 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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:50:01.98 +08:25:23.6 ;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-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20_00sec_-15_00C_LIGHT_0238_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20_00sec_-15_00C_LIGHT_0237_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-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20_00sec_-15_00C_LIGHT_0238_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20_00sec_-15_00C_LIGHT_0237_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,2461082.7586,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260211.2586 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:36:01.09 +04:21:59.6 ;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-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20_00sec_-15_00C_LIGHT_0238_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20_00sec_-15_00C_LIGHT_0237_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-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20_00sec_-15_00C_LIGHT_0238_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20_00sec_-15_00C_LIGHT_0237_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,2461082.7586,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260211.2586 14.12CV 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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:29:58.63 +01:39:18.7 ;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-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20_00sec_-15_00C_LIGHT_0238_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20_00sec_-15_00C_LIGHT_0237_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-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20_00sec_-15_00C_LIGHT_0238_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20_00sec_-15_00C_LIGHT_0237_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
First image: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Last image: 2461082.75882054 11.02.2026 06:12:32.095 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
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): 7769
Objects passed selection criteria: 7764
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 7574
Average stars matched: 7353 (97.0821 %)
Memory usage VmPeak: 113600 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Tue Feb 10 15:05:05 CST 2026
VaST build number 1.0rc88-299-g877bacc0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 00:19:38 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
First image: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Last image: 2461082.75882054 11.02.2026 06:12:32.095 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 175
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.47
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: 16 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): 49959
Objects passed selection criteria: 49825
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 48497.5
Average stars matched: 46738.5 (96.373 %)
Memory usage VmPeak: 148908 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Tue Feb 10 15:05:05 CST 2026
VaST build number 1.0rc88-299-g877bacc0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 00:20:47 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
SExtractor catalog cache: saved Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.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: 2461082.75828741
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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits exists and is non-empty
Saving wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits to local_wcs_cache/
'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits' -> 'local_wcs_cache/wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits'
wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits exists and is non-empty
Saving wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits to local_wcs_cache/
'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits' -> 'local_wcs_cache/wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits'
wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits'
wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.346 +06:00:05.80
Second-epoch image center 09:25:42.193 +05:59:54.85
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:43.346 +06:00:05.80
Second-epoch image center 09:25:39.833 +06:00:11.02
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:25:42.193 +05:59:54.85
Second-epoch second image center 09:25:39.833 +06:00:11.02
Angular distance between the image centers 0.01076 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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits &> /tmp/tmp.iA4gbAlPwA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits &> /tmp/tmp.aebdAFpCu1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits &> /tmp/tmp.mfd8UJkssU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits &> /tmp/tmp.0SxdhJF6u8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
Found non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
The reference image (wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits) and catalog (wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat) found
'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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 4890 out of 7575 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.831362
a=0.000000 b=1.000000 c=22.831362
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.09
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
2.0 pix Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
2.1 pix fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
2.0 pix fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
Limiting magnitude estimates:
15.1 mag. Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
15.1 mag. Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
15.1 mag. fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
15.1 mag. fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.iA4gbAlPwA (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_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits' -> 'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS-calibrated image found: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Checking if the catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS catalog name: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=564, passed=7575
Got 7575 stars (including 6996 good ones) from the SExtractor catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
util/solve_plate_with_UCAC5 got 7575 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 935 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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits -region wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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.aebdAFpCu1 (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_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.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-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits' -> 'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS-calibrated image found: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Checking if the catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS catalog name: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=571, passed=7669
Got 7669 stars (including 7088 good ones) from the SExtractor catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 7669 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
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: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 934 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-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits -region wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.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.mfd8UJkssU (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_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.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_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
Checking if the catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
WCS catalog name: wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=549, passed=7722
Got 7722 stars (including 7156 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits.cat
util/solve_plate_with_UCAC5 got 7722 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 939 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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits -region wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.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.0SxdhJF6u8 (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_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.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_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
Checking if the catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
WCS catalog name: wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=571, passed=7588
Got 7588 stars (including 7001 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits.cat
util/solve_plate_with_UCAC5 got 7588 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 932 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits -region wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.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_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits'
Preparing the HTML report for the field Hya-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20499.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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 20493_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 20493_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:08:59.25 +09:35:41.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20495_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 20495_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 08:55:32.82 +06:09:57.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20499_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 20499_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:25:46.02 +05:17:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.718 3852214922935155200 141.44222730661 +05.28445787737 12.0044 11.6000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20500_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 20500_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:22:27.49 +03:29:35.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Hya-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
SExtractor catalog cache: saved Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Creating symlink local_wcs_cache/wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits exists and is non-empty
wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits exists and is non-empty
wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits exists and is non-empty
wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.346 +06:00:05.80
Second-epoch image center 09:25:42.193 +05:59:54.85
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:43.346 +06:00:05.80
Second-epoch image center 09:25:39.833 +06:00:11.02
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:25:42.193 +05:59:54.85
Second-epoch second image center 09:25:39.833 +06:00:11.02
Angular distance between the image centers 0.01076 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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits &> /tmp/tmp.ONWHyvnEoH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits &> /tmp/tmp.4VbnmcWVpN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits &> /tmp/tmp.I0tqjTPecE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits &> /tmp/tmp.vuMDlp64cI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
Found non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
The reference image (wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits) and catalog (wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat) found
'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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 5118 out of 48659 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.698635
a=0.000000 b=1.000000 c=22.698635
From vast_summary.log: estimated ref. image limiting mag.: -7.47
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 45 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
1.9 pix Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
1.9 pix fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
1.8 pix fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
Limiting magnitude estimates:
15.2 mag. Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
15.2 mag. Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
15.2 mag. fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
15.2 mag. fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ONWHyvnEoH (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_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits' -> 'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS-calibrated image found: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Checking if the catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS catalog name: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2287, passed=48648
Got 48648 stars (including 46264 good ones) from the SExtractor catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
util/solve_plate_with_UCAC5 got 48648 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
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-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits -region wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.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.4VbnmcWVpN (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_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.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-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits' -> 'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS-calibrated image found: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Checking if the catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS catalog name: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2205, passed=48320
Got 48320 stars (including 46022 good ones) from the SExtractor catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 48320 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
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: 0.32"
Estimated accuracy of the plate solution: 0.32"
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-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits -region wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.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.I0tqjTPecE (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_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.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_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
Checking if the catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
WCS catalog name: wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=2369, passed=48865
Got 48865 stars (including 46410 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits.cat
util/solve_plate_with_UCAC5 got 48865 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits -region wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.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.vuMDlp64cI (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_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.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_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
Checking if the catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
WCS catalog name: wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2273, passed=49517
Got 49517 stars (including 47137 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits.cat
util/solve_plate_with_UCAC5 got 49517 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 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-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits -region wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.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_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.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_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-11-46_20.00sec_-15.00C_LIGHT_0237.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.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_2026-02-11_CI_Hya-02-Q1b1x1_001727_TTUQ1b1x1_16518_ufuScIKD/wcs_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238.fits
Preparing the HTML report for the field Hya-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53423.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 53356_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53356_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:07:17.93 +02:09:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.816 577235499980058496 136.82508926305 +02.15272439724 14.3890 13.9353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53357_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53357_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:13:27.69 +06:45:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 1.606 586893090426883840 138.36582164138 +06.76503509829 14.4113 13.9070 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53363_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53363_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:45:54.88 +02:38:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53364_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53364_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 08:56:58.33 +09:52:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 1.760 597556605164722944 134.24351080462 +09.87596532818 14.1923 13.7317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53370_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53370_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:32:46.09 +07:39:42.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)
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Considering the candidate 53373_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53373_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:08:19.90 +02:59:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.723 577492888780292992 137.08338986947 +02.99235360190 13.5571 13.0076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.723#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53374_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53374_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:02:24.38 +03:07:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53375_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53375_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:05:35.21 +04:08:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.476 579873400173338112 136.39734183839 +04.14735499223 13.6451 13.0174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53376_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53376_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:14:37.99 +01:15:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53377_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53377_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:29:14.86 +03:20:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 1.296 3844926092851249152 142.31224825825 +03.33744206067 13.1692 12.7110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53378_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53378_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:56:08.26 +01:26:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53381_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53381_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 08:57:32.03 +05:02:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53386_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
Preparing report for the candidate 53386_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
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Considering the candidate 53391_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53391_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:54:35.74 +01:12:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 1.791 3834589515319110144 148.64939474695 +01.20002886911 13.1275 12.6360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53392_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53392_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:10:45.01 +06:21:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.344 580848770066513664 137.68790223189 +06.36563206430 12.8084 12.3112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53399_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
Preparing report for the candidate 53399_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
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Considering the candidate 53401_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
Preparing report for the candidate 53401_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
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Considering the candidate 53403_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
Preparing report for the candidate 53403_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
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Considering the candidate 53406_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53406_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:08:09.00 +08:25:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53410_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53410_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:02:01.22 +05:05:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 2.697 580248260623869952 135.50580013655 +05.08613461475 14.1049 13.5839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53423_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
Preparing report for the candidate 53423_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
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Considering the candidate 53424_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53424_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:01:05.05 +05:50:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53425_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53425_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:50:53.44 +11:05:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53427_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53427_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:53:08.92 +01:12:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53434_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53434_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:50:56.08 +09:02:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53435_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53435_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:55:42.44 +03:09:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 2.553 3848437447658589824 148.92754279382 +03.16613177147 14.5298 14.0347 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53436_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53436_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:03:26.20 +05:08:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.632 580242114525877376 135.85955064249 +05.14264528771 14.6274 14.1778 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53442_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53442_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:55:09.78 +03:36:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.320 3848657457358750848 148.79097244267 +03.60215260039 14.6486 14.1929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53444_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53444_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:54:19.43 +05:31:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.922 3850117196483637120 148.58115284494 +05.52811012754 14.5331 14.0475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53448_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53448_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:50:27.96 +09:00:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53451_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53451_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:49:28.74 +05:59:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53453_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53453_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:53:11.35 +03:27:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 3.197 3848639929597108736 148.29817967045 +03.46022125419 14.5854 13.9261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53460_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53460_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:38:11.79 +01:57:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53464_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53464_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:56:26.11 +05:50:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 2.376 3850150387990883840 149.10940801534 +05.83753327452 14.5719 14.0427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53469_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53469_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:24:55.94 +01:01:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53470_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53470_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:52:11.20 +01:05:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53471_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53471_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:53:24.10 +04:33:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53472_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53472_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:55:29.82 +01:58:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 2.607 3834797804052977664 148.87495177956 +01.97020872660 14.5387 13.9499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53477_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53477_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:03:54.45 +08:40:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.057 585162738297676800 135.97710602950 +08.66923226954 14.6026 14.0169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53486_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53486_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:55:03.91 +02:53:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53494_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53494_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:52:36.22 +09:52:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53506_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53506_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:56:16.12 +02:09:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 2.528 3834807184261541760 149.06786822842 +02.16220998808 14.4709 13.9700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53510_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 53510_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:56:13.33 +04:22:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 2.575 3848860660851476864 149.05625253199 +04.37412514857 14.4058 13.9098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 38235_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 38235_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks
**** FOUND 09:08:59.27 +09:35:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50567_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238
The candidate 50567_fd_Hya-02-Q1b1x1_2026-02-11_00-12-32_20.00sec_-15.00C_LIGHT_0238 did not pass the final checks