This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0
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,2461120.6858,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260321.1858 11.23CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:53:59.95 +06:30:14.4 ;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-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20_00sec_-15_00C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20_00sec_-15_00C_LIGHT_0159_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20_00sec_-14_90C_LIGHT_0158_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,2461120.6858,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260321.1858 12.60CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:40:14.00 +03:32:36.9 ;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-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20_00sec_-15_00C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20_00sec_-15_00C_LIGHT_0159_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20_00sec_-14_90C_LIGHT_0158_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,2461120.6858,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260321.1858 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:40:57.27 +04:49:19.5 ;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-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20_00sec_-15_00C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20_00sec_-15_00C_LIGHT_0159_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20_00sec_-14_90C_LIGHT_0158_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,2461120.6858,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260321.1858 14.34CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:00:44.09 +05:11:06.5 ;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-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20_00sec_-15_00C_LIGHT_0159_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20_00sec_-14_90C_LIGHT_0158_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20_00sec_-15_00C_LIGHT_0159_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20_00sec_-14_90C_LIGHT_0158_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: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
First image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Last image: 2461120.68607843 21.03.2026 04:27:47.176 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
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: 7 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): 12336
Objects passed selection criteria: 12330
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: 11872
Average stars matched: 11613.2 (97.8205 %)
Memory usage VmPeak: 118256 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 23:31:28 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
First image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Last image: 2461120.68607843 21.03.2026 04:27:47.176 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 235
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
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: 46 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): 75921
Objects passed selection criteria: 75747
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 73034.8
Average stars matched: 70275.2 (96.2217 %)
Memory usage VmPeak: 2091116 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 23:33:24 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.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: 2461120.68552683
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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits exists and is non-empty
Saving wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits to local_wcs_cache/
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits exists and is non-empty
Saving wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits to local_wcs_cache/
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits exists and is non-empty
Saving wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits to local_wcs_cache/
'wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits' -> 'local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits'
wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits exists and is non-empty
Saving wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits to local_wcs_cache/
'wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits' -> 'local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:25.831 +06:00:07.68
Angular distance between the image centers 0.04 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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:24.031 +06:00:02.95
Angular distance between the image centers 0.03 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 08:34:25.831 +06:00:07.68
Second-epoch second image center 08:34:24.031 +06:00:02.95
Angular distance between the image centers 0.00757 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits &> /tmp/tmp.ClELHLg93R
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits &> /tmp/tmp.QXIjFi8XTa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits &> /tmp/tmp.bFvHZFhRJo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits &> /tmp/tmp.LvfPpdityM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
The reference image (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits) and catalog (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat) found
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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 7589 out of 15650 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.955413
a=0.000000 b=1.000000 c=22.955413
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.33
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.33
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
2.3 pix Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
2.3 pix fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
2.3 pix fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
Limiting magnitude estimates:
15.3 mag. Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
15.3 mag. Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
15.2 mag. fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
15.2 mag. fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.2 (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.ClELHLg93R (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1186, passed=15650
Got 15650 stars (including 14444 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 15650 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 953 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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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.QXIjFi8XTa (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1188, passed=15565
Got 15565 stars (including 14349 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 15565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 954 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: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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.bFvHZFhRJo (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1106, passed=14942
Got 14942 stars (including 13828 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits.cat
util/solve_plate_with_UCAC5 got 14942 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.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.LvfPpdityM (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1111, passed=14899
Got 14899 stars (including 13773 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat
util/solve_plate_with_UCAC5 got 14899 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 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: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
Saving fully-calibrated image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits'
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits'
Preparing the HTML report for the field Hya-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out20669.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out20625.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20614_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 20614_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:35:01.81 +02:59:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20625_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
Preparing report for the candidate 20625_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
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Considering the candidate 20628_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 20628_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:17:38.84 +09:10:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 1.289 600393070286747648 124.41163257585 +09.17663158063 11.7035 11.0577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20641_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 20641_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:47:06.93 +08:35:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20643_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 20643_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:47:22.86 +02:18:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20657_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 20657_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:44:55.92 +10:04:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20669_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 20669_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:52:11.42 +04:28:58.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Hya-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:53:59.95 +06:30:14.4
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Creating symlink local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits exists and is non-empty
wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits exists and is non-empty
wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits exists and is non-empty
wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:25.831 +06:00:07.68
Angular distance between the image centers 0.04 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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:24.031 +06:00:02.95
Angular distance between the image centers 0.03 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 08:34:25.831 +06:00:07.68
Second-epoch second image center 08:34:24.031 +06:00:02.95
Angular distance between the image centers 0.00757 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits &> /tmp/tmp.UOzEW8th7y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits &> /tmp/tmp.JnBvZBOSkH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits &> /tmp/tmp.CPdoQ8XdUB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits &> /tmp/tmp.9N8Qz2UWvW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
The reference image (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits) and catalog (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat) found
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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 7690 out of 90472 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.847783
a=0.000000 b=1.000000 c=22.847783
From vast_summary.log: estimated ref. image limiting mag.: -7.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 52 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
2.1 pix Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
2.2 pix fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
2.2 pix fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
Limiting magnitude estimates:
15.5 mag. Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
15.5 mag. Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
15.4 mag. fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
15.4 mag. fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
All-image limiting magnitude estimate: 15.4 (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.UOzEW8th7y (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=6373, passed=90453
Got 90453 stars (including 83928 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 90453 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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.JnBvZBOSkH (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=6475, passed=90928
Got 90928 stars (including 84300 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 90928 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 947 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: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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.CPdoQ8XdUB (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=6415, passed=84826
Got 84826 stars (including 78313 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits.cat
util/solve_plate_with_UCAC5 got 84826 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.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.9N8Qz2UWvW (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=6392, passed=86051
Got 86051 stars (including 79543 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat
util/solve_plate_with_UCAC5 got 86051 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Saving fully-calibrated image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-26-59_20.00sec_-14.90C_LIGHT_0158.fits
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Hya-01-Q2b1x1_232825_TTUQ2b1x1_5408_G4S3SvA0/wcs_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159.fits
Preparing the HTML report for the field Hya-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out106171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out106341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106805.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
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: 2s
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Considering the candidate 106171_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106171_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:53:43.20 +03:44:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.362 581544932725757952 133.42962098991 +03.74931150925 14.4294 13.8688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106196_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106196_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:33:01.69 +02:11:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.594 3079551891228910848 128.25699279565 +02.18760206230 14.3809 13.7310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106203_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106203_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:49:24.86 +02:42:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106207_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106207_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:24:57.95 +04:23:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.723 3092247333519245184 126.24103957827 +04.39384489527 14.5377 13.9557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.723#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106216_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106216_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:10:58.97 +02:07:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.202 3090759591208717952 122.74601892550 +02.11734892099 14.4770 14.0741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.202#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106220_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106220_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:11:16.44 +04:13:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 1.245 3094586097833058688 122.81818534588 +04.21986733860 14.2303 13.7257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106226_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106226_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:38:12.65 +03:34:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106231_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106231_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:38:49.61 +06:11:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 2.592 594720483640587648 129.70614236801 +06.19653237127 14.1187 13.6210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106233_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106233_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:10:58.52 +05:07:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.091 3094993844848876416 122.74367102881 +05.13211731792 13.8764 13.4216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106235_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106235_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:11:34.82 +05:06:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 0.745 3094806515553431168 122.89505104379 +05.11225989716 13.9728 13.4832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106236_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106236_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:58:28.98 +02:32:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106237_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106237_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:15:36.67 +01:57:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 2.363 3090000103551585920 123.90214180365 +01.95037192792 14.0065 13.5268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106238_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106238_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:22:32.71 +08:12:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 0.724 599333347236879360 125.63643451938 +08.20597646303 13.6434 13.2094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106242_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106242_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:19:13.76 +10:01:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106243_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106243_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:59:59.61 +02:15:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106245_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106245_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:37:10.81 +04:50:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.688 594476593922306688 129.29472574540 +04.84984739087 13.2942 12.8500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106246_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106246_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:16:10.03 +02:00:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.837 3089961139608252544 124.04104397777 +02.01383362452 13.3198 12.8745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106250_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106250_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:52:44.12 +09:44:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.257 597638209543645440 133.18357586572 +09.74018435250 13.1445 12.6474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106252_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106252_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:18:44.84 +01:57:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106258_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106258_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:28:07.89 +02:49:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.370 3091759146061150336 127.03270010591 +02.82181017799 12.7691 12.3132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106262_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106262_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:27:29.35 +04:26:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 1.734 3092213519241165824 126.87246586373 +04.44250471635 12.3707 12.0047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106265_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106265_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:10:05.48 +06:20:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106291_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106291_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:53:59.97 +06:30:14.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 106303_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106303_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:29:00.68 +06:54:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.789 595909223213710336 127.25282079899 +06.91238554014 12.1364 11.7208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106317_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106317_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:19:12.20 +05:42:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.046 3096400768756975872 124.80079619062 +05.71101042121 12.4132 11.7035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106341_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
Preparing report for the candidate 106341_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
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Considering the candidate 106445_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106445_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:11:34.92 +02:34:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.339 3090859371888726016 122.89577226978 +02.58180931809 13.3652 12.7038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106459_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106459_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:55:33.34 +05:55:25.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 106475_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
Preparing report for the candidate 106475_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
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Considering the candidate 106520_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106520_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:21:06.51 +09:47:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 4.782 600530887198673536 125.27735381442 +09.78969792617 13.7626 12.9480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106523_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106523_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:21:39.23 +02:41:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.254 3090467155475022080 125.41298155043 +02.69762886265 13.7714 13.2219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106554_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106554_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:21:16.60 +08:23:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.327 599353378964218112 125.31917221197 +08.39447949036 14.1066 13.6150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106569_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106569_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:10:37.15 +03:49:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106572_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106572_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:12:55.38 +04:07:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 2.265 3091670124275497728 123.23078668934 +04.13262805780 14.2010 13.6986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106582_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106582_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:10:23.98 +05:01:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 0.475 3094969174556754304 122.59981600535 +05.01891915675 14.1479 13.6440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106589_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106589_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:11:55.73 +03:25:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.808 3091471284470139648 122.98229462526 +03.42738370754 14.3810 13.8575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106593_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106593_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:19:13.89 +02:09:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 2.720 3090349473371265792 124.80739181221 +02.15866452378 14.1805 13.6309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106598_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106598_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:12:11.14 +05:41:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 2.003 3096532611371325184 123.04595101116 +05.69536375364 14.0255 13.4368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.003#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106602_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106602_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:16:04.69 +03:28:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 1.727 3091375764396283136 124.01915091935 +03.47969600640 14.2299 13.6612 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106605_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106605_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:10:47.00 +03:38:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.124 3091536842850703488 122.69554912245 +03.63565825022 14.2378 13.7760 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106624_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106624_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:13:31.81 +05:11:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.222 3096297144082778880 123.38234241302 +05.19716429080 14.2658 13.6546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106652_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106652_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:11:30.58 +05:54:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.132 3096586281282633984 122.87713368604 +05.90105701153 14.2279 13.7782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106667_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106667_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:19:28.86 +06:16:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.564 3096810920954717696 124.86983838327 +06.27692412049 14.3864 13.8904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106676_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106676_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:29:27.68 +04:26:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 1.677 3092578973713226368 127.36493393065 +04.44821413837 14.8494 13.7390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106683_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106683_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:10:51.65 +04:28:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 2.545 3094700069084384256 122.71591710311 +04.48002364118 14.7277 14.2417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106692_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106692_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:20:21.86 +06:40:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.009 3096897786669203584 125.09114832387 +06.68007843174 14.5077 14.1077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106739_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106739_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:12:20.57 +01:51:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 3.636 3090736845062165248 123.08670157170 +01.86632526529 14.5044 14.0856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106756_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106756_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:41:48.58 +02:36:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.265 3079123764593515392 130.45218070613 +02.60773274603 14.3975 13.7357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106777_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106777_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:15:35.16 +03:04:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 4.714 3091219118349284480 123.89525171702 +03.07867933435 14.6615 14.1980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106788_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 106788_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks
**** FOUND 08:14:49.06 +02:23:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.759 3090783127629771520 123.70455872538 +02.39121145094 14.6826 14.3142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106805_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
Preparing report for the candidate 106805_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
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Considering the candidate 78550_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159
The candidate 78550_fd_Hya-01-Q2b1x1_2026-03-20_23-27-47_20.00sec_-15.00C_LIGHT_0159 did not pass the final checks