This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S
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,2461093.7108,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2108 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:22.18 +01:32:43.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20_00sec_-15_00C_LIGHT_0190_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20_00sec_-15_00C_LIGHT_0189_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20_00sec_-15_00C_LIGHT_0189_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2108* 09 42 06.38 +09 43 14.9 13.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7108,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2108 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:42:06.38 +09:43:14.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20_00sec_-15_00C_LIGHT_0190_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20_00sec_-15_00C_LIGHT_0189_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20_00sec_-15_00C_LIGHT_0189_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,2461093.7108,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2108 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:27:46.07 +05:32:18.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20_00sec_-15_00C_LIGHT_0190_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20_00sec_-15_00C_LIGHT_0189_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20_00sec_-15_00C_LIGHT_0189_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,2461093.7108,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.2108 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:19:20.38 +02:35:30.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20_00sec_-15_00C_LIGHT_0190_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20_00sec_-15_00C_LIGHT_0189_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20_00sec_-15_00C_LIGHT_0190_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20_00sec_-15_00C_LIGHT_0221_fits__*pix.png resample_wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20_00sec_-15_00C_LIGHT_0189_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
First image: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Last image: 2461093.71105872 22.02.2026 05:03:45.473 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 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): 8358
Objects passed selection criteria: 8353
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: 8034.75
Average stars matched: 7624.75 (94.8972 %)
Memory usage VmPeak: 114060 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Feb 21 23:09:26 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
First image: 2461049.73278426 09.01.2026 05:35:02.560 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Last image: 2461093.71105872 22.02.2026 05:03:45.473 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 262
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.47
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 48 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): 52397
Objects passed selection criteria: 52269
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: 50447.8
Average stars matched: 47887.8 (94.9254 %)
Memory usage VmPeak: 151668 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Feb 21 23:12:23 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
SExtractor catalog cache: saved Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.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: 2461093.71059308
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits exists and is non-empty
Saving wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits to local_wcs_cache/
'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits' -> 'local_wcs_cache/wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits'
wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits exists and is non-empty
Saving wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits to local_wcs_cache/
'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits' -> 'local_wcs_cache/wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits'
wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits'
wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits exists and is non-empty
Saving wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.346 +06:00:05.80
Second-epoch image center 09:26:05.780 +06:00:25.95
Angular distance between the image centers 0.09 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:43.346 +06:00:05.80
Second-epoch image center 09:26:08.447 +06:00:30.99
Angular distance between the image centers 0.10 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:26:05.780 +06:00:25.95
Second-epoch second image center 09:26:08.447 +06:00:30.99
Angular distance between the image centers 0.01114 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits &> /tmp/tmp.5WyHDfwVA8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits &> /tmp/tmp.Z4mEbgsYwm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits &> /tmp/tmp.c81AU3SOcR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits &> /tmp/tmp.uOw95BiBw2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
Found non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
The reference image (wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits) and catalog (wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat) found
'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 4890 out of 7575 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.831362
a=0.000000 b=1.000000 c=22.831362
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.09
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
2.0 pix Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
2.1 pix fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
2.1 pix fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
Limiting magnitude estimates:
15.1 mag. Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
15.1 mag. Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
15.2 mag. fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
15.2 mag. fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5WyHDfwVA8 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits' -> 'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS-calibrated image found: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Checking if the catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS catalog name: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=564, passed=7575
Got 7575 stars (including 6996 good ones) from the SExtractor catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
util/solve_plate_with_UCAC5 got 7575 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 935 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits -region wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Z4mEbgsYwm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits' -> 'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS-calibrated image found: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Checking if the catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS catalog name: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=571, passed=7669
Got 7669 stars (including 7088 good ones) from the SExtractor catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 7669 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 934 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits -region wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.c81AU3SOcR (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
Checking if the catalog wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
WCS catalog name: wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=705, passed=8589
Got 8589 stars (including 7874 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits.cat
util/solve_plate_with_UCAC5 got 8589 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 934 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits -region wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.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.uOw95BiBw2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
Checking if the catalog wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
WCS catalog name: wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=687, passed=8566
Got 8566 stars (including 7869 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat
util/solve_plate_with_UCAC5 got 8566 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits -region wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits'
Preparing the HTML report for the field Hya-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20511.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 20511_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
Preparing report for the candidate 20511_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
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Considering the candidate 20526_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 20526_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:08:59.24 +09:35:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20530_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 20530_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:23:37.36 +05:10:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20531_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 20531_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 08:55:32.81 +06:09:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20532_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 20532_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:22:31.69 +06:19:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20533_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 20533_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:22:27.44 +03:29:35.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20535_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 20535_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:25:46.05 +05:17:03.8 in the exclusion list exclusion_list.txt ****
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-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
09:07:22.18 +01:32:43.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
SExtractor catalog cache: saved Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Creating symlink local_wcs_cache/wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits exists and is non-empty
wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits exists and is non-empty
wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits exists and is non-empty
wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.346 +06:00:05.80
Second-epoch image center 09:26:05.780 +06:00:25.95
Angular distance between the image centers 0.09 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:43.346 +06:00:05.80
Second-epoch image center 09:26:08.447 +06:00:30.99
Angular distance between the image centers 0.10 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:26:05.780 +06:00:25.95
Second-epoch second image center 09:26:08.447 +06:00:30.99
Angular distance between the image centers 0.01114 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits &> /tmp/tmp.KTTXuGK62R
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits &> /tmp/tmp.D1d2ztSuWb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits &> /tmp/tmp.bpQAt9KsbG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits &> /tmp/tmp.5zbVzxP6z6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
Found non-empty wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits and wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
The reference image (wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits) and catalog (wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat) found
'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5118 out of 48659 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.698635
a=0.000000 b=1.000000 c=22.698635
From vast_summary.log: estimated ref. image limiting mag.: -7.47
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 37 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
1.9 pix Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
1.9 pix fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
1.9 pix fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
Limiting magnitude estimates:
15.2 mag. Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
15.2 mag. Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
15.4 mag. fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
15.4 mag. fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.6 (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.KTTXuGK62R (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits' -> 'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS-calibrated image found: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
Checking if the catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits
WCS catalog name: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2287, passed=48648
Got 48648 stars (including 46264 good ones) from the SExtractor catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat
util/solve_plate_with_UCAC5 got 48648 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits -region wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-02_20.00sec_-15.00C_LIGHT_0221.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.D1d2ztSuWb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits' -> 'wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS-calibrated image found: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
Checking if the catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits
WCS catalog name: wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2205, passed=48320
Got 48320 stars (including 46022 good ones) from the SExtractor catalog wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 48320 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits -region wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q1b1x1_2026-01-08_23-35-58_20.00sec_-15.00C_LIGHT_0222.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bpQAt9KsbG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
Checking if the catalog wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
WCS catalog name: wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=2919, passed=53302
Got 53302 stars (including 50288 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits.cat
util/solve_plate_with_UCAC5 got 53302 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits -region wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.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.5zbVzxP6z6 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
Checking if the catalog wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat corresponding to the image wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
WCS catalog name: wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=2878, passed=53002
Got 53002 stars (including 50028 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat
util/solve_plate_with_UCAC5 got 53002 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits -region wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-05_20.00sec_-15.00C_LIGHT_0189.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-02-Q1b1x1_230421_TTUQ1b1x1_16526_FCvug49S/wcs_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190.fits
Preparing the HTML report for the field Hya-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out53626.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out53509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53552.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53372_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53372_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:07:17.90 +02:09:10.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53373_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53373_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:13:27.65 +06:45:54.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53374_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53374_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 08:58:04.59 +02:57:03.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53376_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53376_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:45:55.02 +02:38:52.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53385_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53385_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:01:07.97 +02:32:19.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53393_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53393_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:56:08.26 +01:26:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53395_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53395_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:42:41.83 +08:07:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53415_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53415_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:07:22.18 +01:32:43.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53509_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
Preparing report for the candidate 53509_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
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Considering the candidate 53516_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
Preparing report for the candidate 53516_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
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Considering the candidate 53552_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
Preparing report for the candidate 53552_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
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Considering the candidate 53558_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53558_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:50:53.41 +11:05:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53576_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53576_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:00:19.18 +03:30:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53584_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53584_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:56:07.07 +06:31:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53594_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53594_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:01:05.01 +05:50:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53599_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53599_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:50:36.38 +09:59:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 1.674 3879175502099635072 147.65190469859 +09.99417388258 14.5528 14.0381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53601_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53601_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:50:56.08 +09:02:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53604_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53604_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:52:04.63 +03:11:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53609_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53609_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:56:13.38 +04:22:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53610_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53610_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:55:29.58 +02:58:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53615_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53615_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:46:00.90 +09:14:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53617_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53617_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:56:49.46 +06:51:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53618_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53618_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:53:08.86 +01:12:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53619_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53619_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:54:57.65 +01:33:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 2.091 3834745336732508288 148.74078892145 +01.55121558262 14.7523 14.1506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53625_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53625_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:51:08.33 +04:18:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 0.975 3849560190764925184 147.78497953285 +04.31642888632 14.6305 14.1229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53626_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53626_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:49:08.44 +02:28:52.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)
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Considering the candidate 53629_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53629_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 08:57:31.76 +05:03:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 3.484 581787203240757120 134.38287543054 +05.05780298642 14.6033 13.9941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53637_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53637_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 08:58:25.77 +06:55:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53647_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53647_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:53:23.95 +04:33:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53649_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53649_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:54:04.20 +11:06:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.718 3879689077108804736 148.51798624301 +11.11279771446 14.5497 14.1095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53650_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53650_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:48:10.53 +07:43:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.810 3853907006905992448 147.04437967375 +07.72183086353 14.4673 13.7226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53652_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53652_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:47:35.09 +04:34:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 0.252 3849764184531624448 146.89626272319 +04.58257203695 14.7557 14.2262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53656_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53656_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:56:16.13 +02:09:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53660_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53660_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 08:55:30.97 +05:26:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53706_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53706_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:50:34.80 +04:46:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53708_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 53708_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks
**** FOUND 09:52:36.09 +09:52:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38235_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190
The candidate 38235_fd_Hya-02-Q1b1x1_2026-02-21_23-03-45_20.00sec_-15.00C_LIGHT_0190 did not pass the final checks