This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu
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,2461082.7547,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260211.2547 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:16:25.00 -00:17:44.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_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,2461082.7547,12.11,0.05,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 20260211.2547 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:14.02 +00:29:38.3 ;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-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_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,2461082.7547,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260211.2547 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:00:08.24 +02:03:55.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_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
WW Hya,2461082.7547,11.10,0.05,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
WW Hya 20260211.2547 11.10CV 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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:57:46.71 -03:16:53.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_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,2461082.7547,12.88,0.05,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 20260211.2547 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:32:15.66 -05:34:16.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_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 11.2547* 09 55 47.14 -01 33 47.1 13.6 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461082.7547,13.59,0.05,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 20260211.2547 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:55:47.14 -01:33:47.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_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,2461082.7547,14.04,0.05,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 20260211.2547 14.04CV 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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:29:58.99 +01:39:18.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_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
RZ Hya,2461082.7547,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RZ Hya 20260211.2547 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:24:50.37 -06:47:31.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20_00sec_-15_00C_LIGHT_0231_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.90316561 23.12.2025 09:40:23.509 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
First image: 2461032.90316561 23.12.2025 09:40:23.509 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Last image: 2461082.75498444 11.02.2026 06:07:00.656 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 10203
Objects passed selection criteria: 10199
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: 9858
Average stars matched: 9688.75 (98.2831 %)
Memory usage VmPeak: 115780 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 00:14:50 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: 2461032.90316561 23.12.2025 09:40:23.509 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
First image: 2461032.90316561 23.12.2025 09:40:23.509 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Last image: 2461082.75498444 11.02.2026 06:07:00.656 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 172
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.39
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: 23 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): 65132
Objects passed selection criteria: 64993
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: 63057.2
Average stars matched: 60940.5 (96.6431 %)
Memory usage VmPeak: 168668 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 00:16:07 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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
SExtractor catalog cache: saved Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat to cache
SExtractor catalog cache: saved Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.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: 2461082.75449899
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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits exists and is non-empty
Saving wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits to local_wcs_cache/
'wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits' -> 'local_wcs_cache/wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits'
wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits exists and is non-empty
Saving wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits to local_wcs_cache/
'wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits' -> 'local_wcs_cache/wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits'
wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits exists and is non-empty
Saving wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits to local_wcs_cache/
'wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits' -> 'local_wcs_cache/wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits'
wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
Saving wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits to local_wcs_cache/
'wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits' -> 'local_wcs_cache/wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.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 09:25:43.993 -02:00:09.35
Second-epoch image center 09:25:49.999 -01:59:37.72
Angular distance between the image centers 0.03 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 09:25:43.993 -02:00:09.35
Second-epoch image center 09:25:52.785 -01:59:53.94
Angular distance between the image centers 0.04 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 09:25:49.999 -01:59:37.72
Second-epoch second image center 09:25:52.785 -01:59:53.94
Angular distance between the image centers 0.01244 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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits &> /tmp/tmp.UudZ7Xd3j0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits &> /tmp/tmp.DZndtR5yNh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits &> /tmp/tmp.OE4UvazqNy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.soFc1320bL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
Found non-empty wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
The reference image (wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits) and catalog (wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat) found
'wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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 5565 out of 10420 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.932573
a=0.000000 b=1.000000 c=22.932573
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
2.0 pix Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
2.0 pix fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
2.0 pix fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
Limiting magnitude estimates:
15.3 mag. Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
15.3 mag. Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
15.2 mag. fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
15.2 mag. fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.UudZ7Xd3j0 (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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits' -> 'wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS-calibrated image found: wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Checking if the catalog wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat corresponding to the image wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat corresponding to the image wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS catalog name: wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=740, passed=10420
Got 10420 stars (including 9668 good ones) from the SExtractor catalog wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
util/solve_plate_with_UCAC5 got 10420 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 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_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits -region wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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.DZndtR5yNh (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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits' -> 'wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS-calibrated image found: wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Checking if the catalog wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS catalog name: wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=743, passed=10444
Got 10444 stars (including 9684 good ones) from the SExtractor catalog wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat
util/solve_plate_with_UCAC5 got 10444 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits -region wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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.OE4UvazqNy (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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
WCS_IMAGE_NAME=wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
WCS-calibrated image found: wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
Checking if the catalog wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits.cat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits.cat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
WCS catalog name: wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=774, passed=9462
Got 9462 stars (including 8673 good ones) from the SExtractor catalog wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits.cat
util/solve_plate_with_UCAC5 got 9462 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.36"
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: 0.33"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits -region wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.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.soFc1320bL (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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=786, passed=9415
Got 9415 stars (including 8615 good ones) from the SExtractor catalog wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 9415 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.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-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits'
Saving fully-calibrated image wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits'
Preparing the HTML report for the field Hya-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out04227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20546.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20529_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
Preparing report for the candidate 20529_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20541_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
Preparing report for the candidate 20541_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20544_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 20544_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:24:50.37 -06:47:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 1.759 5745316492741496320 141.20975797736 -06.79280804443 10.4424 8.8635 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20546_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
Preparing report for the candidate 20546_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04227_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
Preparing report for the candidate 04227_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06636_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 06636_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 08:58:16.53 -00:49:52.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Hya-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:57:46.71 -03:16:53.4
09:16:25.00 -00:17:44.9
09:03:14.02 +00:29:38.3
09:00:08.24 +02:03:55.5
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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
SExtractor catalog cache: saved Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat to cache
SExtractor catalog cache: saved Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Creating symlink local_wcs_cache/wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits exists and is non-empty
wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits exists and is non-empty
wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits exists and is non-empty
wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.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 09:25:43.993 -02:00:09.35
Second-epoch image center 09:25:49.999 -01:59:37.72
Angular distance between the image centers 0.03 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 09:25:43.993 -02:00:09.35
Second-epoch image center 09:25:52.785 -01:59:53.94
Angular distance between the image centers 0.04 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 09:25:49.999 -01:59:37.72
Second-epoch second image center 09:25:52.785 -01:59:53.94
Angular distance between the image centers 0.01244 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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits &> /tmp/tmp.pYcXswq2Lr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits &> /tmp/tmp.5CmCf7xRms
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits &> /tmp/tmp.359L0AHoaO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.ctEtQQbt3u
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
Found non-empty wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
The reference image (wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits) and catalog (wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat) found
'wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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 5627 out of 64348 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.821408
a=0.000000 b=1.000000 c=22.821408
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
____ 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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
1.9 pix Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
1.8 pix fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
1.8 pix fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
Limiting magnitude estimates:
15.4 mag. Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
15.4 mag. Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
15.3 mag. fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
15.3 mag. fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.7 (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.pYcXswq2Lr (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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits' -> 'wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS-calibrated image found: wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Checking if the catalog wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat corresponding to the image wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat corresponding to the image wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS catalog name: wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=3271, passed=64335
Got 64335 stars (including 60948 good ones) from the SExtractor catalog wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
util/solve_plate_with_UCAC5 got 64335 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits -region wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q1b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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.5CmCf7xRms (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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits' -> 'wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS-calibrated image found: wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Checking if the catalog wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS catalog name: wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=3228, passed=64125
Got 64125 stars (including 60786 good ones) from the SExtractor catalog wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat
util/solve_plate_with_UCAC5 got 64125 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits -region wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q1b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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.359L0AHoaO (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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
WCS_IMAGE_NAME=wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
WCS-calibrated image found: wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
Checking if the catalog wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits.cat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits.cat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
WCS catalog name: wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=3334, passed=62389
Got 62389 stars (including 58922 good ones) from the SExtractor catalog wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits.cat
util/solve_plate_with_UCAC5 got 62389 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 942 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 - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits -region wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.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.ctEtQQbt3u (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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=29, blended=3311, passed=63072
Got 63072 stars (including 59646 good ones) from the SExtractor catalog wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 63072 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 941 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
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 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Hya-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.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-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-06-18_20.00sec_-15.00C_LIGHT_0231.fits
Saving fully-calibrated image wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.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-04-Q1b1x1_001124_TTUQ1b1x1_19670_dEHDszHu/wcs_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232.fits
Preparing the HTML report for the field Hya-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out78870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79031.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79036.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79063.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79072.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79129.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out03064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78991.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 78870_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78870_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:45:11.98 -04:29:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.487 3825822284477253248 146.30007078433 -04.48714436619 14.4851 13.9853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78872_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78872_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:37:26.15 -06:08:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78875_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78875_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 08:57:52.94 -00:00:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78876_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78876_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:24:47.87 -06:59:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 2.152 5745297697964616576 141.20005980080 -06.99061125436 14.7125 13.9278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78878_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78878_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:37:07.22 -04:41:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78879_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78879_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 08:59:36.43 +00:16:32.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)
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Considering the candidate 78882_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78882_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:04:50.14 +02:06:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78884_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78884_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:26:08.81 +01:38:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 0.770 3844461411749646848 141.53649613376 +01.64383461855 14.2283 13.7223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78886_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78886_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:53:37.67 +01:03:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78893_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78893_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:49:05.86 -04:41:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.206 3822774571388874368 147.27424657112 -04.69518315840 13.7797 13.3428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.206#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78896_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78896_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:28:22.54 +01:03:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.399 3841002279449207680 142.09401015788 +01.05736509812 13.3645 12.8606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78898_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78898_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:44:13.33 +01:49:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78903_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78903_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:16:25.00 -00:17:44.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 78915_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78915_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:03:14.00 +00:29:38.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 78918_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78918_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:00:13.10 -04:27:55.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)
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Considering the candidate 78920_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78920_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:00:08.21 +02:03:55.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 78936_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
Preparing report for the candidate 78936_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
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Considering the candidate 78940_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78940_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:52:02.55 -00:37:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 2.552 3833733030120923904 148.01099095467 -00.62367059532 13.0463 12.5477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78946_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78946_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:16:46.44 -04:35:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78954_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78954_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:18:11.53 -07:03:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78962_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
Preparing report for the candidate 78962_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
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Considering the candidate 78970_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78970_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:44:50.50 -00:37:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78972_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78972_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:48:20.65 -06:15:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78980_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78980_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 08:55:10.36 -03:14:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.184 5763497261104512000 133.79312367121 -03.23672939131 13.9292 13.4664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78991_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
Preparing report for the candidate 78991_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
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Considering the candidate 78993_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 78993_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:26:14.45 -05:53:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 1.246 5746231045897734784 141.56036588349 -05.89688580416 13.8956 13.2784 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79004_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79004_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:56:51.62 -05:36:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.398 3821743130697992704 149.21470230315 -05.61059123951 14.3552 13.8860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79024_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79024_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:38:11.83 +01:57:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79026_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79026_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:44:27.43 -02:13:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79027_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79027_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:51:13.78 +00:31:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.092 3834165516147657216 147.80799385686 +00.52667836111 14.5594 14.0560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79031_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79031_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:49:38.56 -03:24:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.163 3826014080536760832 147.41088558098 -03.41648806920 14.4319 13.7834 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79036_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79036_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:44:31.64 -06:30:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 0.877 3820827787267890432 146.13204722631 -06.51590877239 14.4134 13.8742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79037_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79037_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:19:45.09 +02:36:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 0.858 3845201967190611072 139.93801162168 +02.60791768226 14.4407 13.8459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79039_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79039_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:08:13.28 +01:15:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79045_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79045_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 08:56:21.88 -06:35:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 2.178 5757197501858401152 134.09131336278 -06.58674619400 14.7069 14.2043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79047_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79047_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:25:55.76 +01:45:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79049_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79049_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:50:53.35 -06:03:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.247 3820176876384077440 147.72235131093 -06.05998008493 14.6673 14.1274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79057_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79057_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:12:40.71 +02:18:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 1.061 3845307520306929792 138.16985723597 +02.30962383819 14.6166 14.1163 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79060_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79060_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:05:55.99 -06:54:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 1.354 5756598989575229568 136.48355422014 -06.91545101549 14.4958 13.8918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79063_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79063_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:12:52.53 +02:48:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 2.002 578750283405837312 138.21838576535 +02.80409909181 14.5716 14.0219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79072_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79072_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 09:05:43.70 -06:22:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.757 5756697881198050176 136.43252667131 -06.37692896142 14.2290 13.6721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79129_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 79129_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 08:55:24.18 -03:10:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 0.983 5763521519079788672 133.85056815688 -03.17537049994 14.6894 14.2366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 03064_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
Preparing report for the candidate 03064_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
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Considering the candidate 25919_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 25919_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks
**** FOUND 08:57:46.71 -03:16:53.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52576_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232
The candidate 52576_fd_Hya-04-Q1b1x1_2026-02-11_00-07-00_20.00sec_-15.00C_LIGHT_0232 did not pass the final checks