This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1673* 05 39 21.43 +06 17 49.3 13.6 U Ori 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,2461093.6673,13.61,0.05,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 20260222.1673 13.61CV 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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:21.43 +06:17:49.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20_00sec_-14_90C_LIGHT_0126_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20_00sec_-15_00C_LIGHT_0125_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20_00sec_-14_90C_LIGHT_0126_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20_00sec_-15_00C_LIGHT_0125_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 22.1673* 05 27 23.83 +09 27 08.3 13.7 U Ori 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,2461093.6673,13.69,0.05,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 20260222.1673 13.69CV 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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:27:23.83 +09:27:08.3 ;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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20_00sec_-14_90C_LIGHT_0126_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20_00sec_-15_00C_LIGHT_0125_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20_00sec_-14_90C_LIGHT_0126_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20_00sec_-15_00C_LIGHT_0125_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 22.1673* 04 57 37.44 +08 51 07.2 14.4 U Ori 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,2461093.6673,14.36,0.05,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 20260222.1673 14.36CV 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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:37.44 +08:51:07.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20_00sec_-14_90C_LIGHT_0126_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20_00sec_-15_00C_LIGHT_0125_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20_00sec_-14_90C_LIGHT_0126_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20_00sec_-14_90C_LIGHT_0326_fits__*pix.png resample_wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20_00sec_-15_00C_LIGHT_0125_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.77884545 23.12.2025 06:41:22.247 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
First image: 2461032.77884545 23.12.2025 06:41:22.247 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
Last image: 2461093.66760568 22.02.2026 04:01:11.131 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 14 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): 16330
Objects passed selection criteria: 16323
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: 15623.5
Average stars matched: 15325.8 (98.0942 %)
Memory usage VmPeak: 120832 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 Sun Feb 22 02:21:45 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.77884545 23.12.2025 06:41:22.247 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
First image: 2461032.77884545 23.12.2025 06:41:22.247 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
Last image: 2461093.66760568 22.02.2026 04:01:11.131 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 207
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
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: 141 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): 105337
Objects passed selection criteria: 105112
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: 100908
Average stars matched: 97589 (96.7113 %)
Memory usage VmPeak: 1930588 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 Sun Feb 22 02:26:46 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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
SExtractor catalog cache: saved Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat to cache
SExtractor catalog cache: saved Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.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: 2461093.66704992
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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits exists and is non-empty
Saving wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits to local_wcs_cache/
'wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits' -> 'local_wcs_cache/wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits'
wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits exists and is non-empty
Saving wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits to local_wcs_cache/
'wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits' -> 'local_wcs_cache/wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits'
wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits exists and is non-empty
Saving wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits to local_wcs_cache/
'wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits' -> 'local_wcs_cache/wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits'
wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits exists and is non-empty
Saving wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits to local_wcs_cache/
'wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits' -> 'local_wcs_cache/wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.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 05:08:17.653 +06:01:42.67
Second-epoch image center 05:08:43.382 +06:00:08.79
Angular distance between the image centers 0.11 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 05:08:17.653 +06:01:42.67
Second-epoch image center 05:08:40.953 +06:00:11.88
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 05:08:43.382 +06:00:08.79
Second-epoch second image center 05:08:40.953 +06:00:11.88
Angular distance between the image centers 0.01010 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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits &> /tmp/tmp.euQ0CpK4TH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits &> /tmp/tmp.2vSGuNqJ6j
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits &> /tmp/tmp.LwH2wyG92S
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits &> /tmp/tmp.tkUZOFNpSU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits and wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits and wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
Found non-empty wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits and wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
The reference image (wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits) and catalog (wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat) found
'wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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 8346 out of 16639 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.941484
a=0.000000 b=1.000000 c=22.941484
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
2.0 pix Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
2.1 pix fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
2.1 pix fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
Limiting magnitude estimates:
15.3 mag. Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
15.3 mag. Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
15.1 mag. fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
15.1 mag. fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
All-image limiting magnitude estimate: 15.1 (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.euQ0CpK4TH (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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits' -> 'wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
WCS-calibrated image found: wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
Checking if the catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
WCS catalog name: wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1525, passed=16639
Got 16639 stars (including 15103 good ones) from the SExtractor catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
util/solve_plate_with_UCAC5 got 16639 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits -region wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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.2vSGuNqJ6j (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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits' -> 'wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
WCS-calibrated image found: wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
Checking if the catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
WCS catalog name: wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1536, passed=16598
Got 16598 stars (including 15044 good ones) from the SExtractor catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat
util/solve_plate_with_UCAC5 got 16598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits -region wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.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.LwH2wyG92S (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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
Checking if the catalog wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
WCS catalog name: wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1339, passed=14994
Got 14994 stars (including 13630 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits.cat
util/solve_plate_with_UCAC5 got 14994 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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
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 954 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: 0.30"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits -region wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.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.tkUZOFNpSU (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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
Checking if the catalog wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
WCS catalog name: wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1382, passed=14663
Got 14663 stars (including 13264 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits.cat
util/solve_plate_with_UCAC5 got 14663 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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
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 954 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: 0.34"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits -region wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.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_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits'
Saving fully-calibrated image wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits'
Preparing the HTML report for the field Ori-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20991.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20849_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 20849_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:30:58.03 +03:45:27.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20862_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 20862_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:37:37.22 +02:19:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20955_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 20955_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:36:21.13 +09:29:27.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20985_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 20985_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:01:08.28 +08:32:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.378 3290270266739540224 075.28443535428 +08.54916661246 12.0020 11.3072 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20991_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 20991_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:28:09.56 +04:14:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.724 3236310324856707840 082.03979710107 +04.24963560849 12.4009 11.9731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21002_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 21002_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:23:30.74 +03:47:30.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Ori-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
SExtractor catalog cache: saved Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat to cache
SExtractor catalog cache: saved Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
Creating symlink local_wcs_cache/wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits exists and is non-empty
wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits exists and is non-empty
wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits exists and is non-empty
wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.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 05:08:17.653 +06:01:42.67
Second-epoch image center 05:08:43.382 +06:00:08.79
Angular distance between the image centers 0.11 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 05:08:17.653 +06:01:42.67
Second-epoch image center 05:08:40.953 +06:00:11.88
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 05:08:43.382 +06:00:08.79
Second-epoch second image center 05:08:40.953 +06:00:11.88
Angular distance between the image centers 0.01010 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/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits &> /tmp/tmp.LHAfrssB1l
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits &> /tmp/tmp.EivhMlRCXy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits &> /tmp/tmp.zgvH8SBx2O
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits &> /tmp/tmp.ZoRPnf6um6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits and wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits and wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
Found non-empty wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits and wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
The reference image (wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits) and catalog (wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat) found
'wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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 8481 out of 106531 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.798883
a=0.000000 b=1.000000 c=22.798883
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 52 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
1.9 pix Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
2.0 pix fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
1.9 pix fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
Limiting magnitude estimates:
15.5 mag. Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
15.5 mag. Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
15.3 mag. fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
15.3 mag. fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
All-image limiting magnitude estimate: 15.3 (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.LHAfrssB1l (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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits' -> 'wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
WCS-calibrated image found: wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
Checking if the catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits
WCS catalog name: wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=9253, passed=106506
Got 106506 stars (including 97096 good ones) from the SExtractor catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat
util/solve_plate_with_UCAC5 got 106506 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 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: 0.32"
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 955 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: 0.31"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits -region wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-41-22_20.00sec_-14.90C_LIGHT_0326.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.EivhMlRCXy (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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits' -> 'wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
WCS-calibrated image found: wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
Checking if the catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat corresponding to the image wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits
WCS catalog name: wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=9240, passed=106589
Got 106589 stars (including 97168 good ones) from the SExtractor catalog wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat
util/solve_plate_with_UCAC5 got 106589 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits -region wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q1b1x1_2025-12-23_00-42-07_20.00sec_-15.00C_LIGHT_0327.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.zgvH8SBx2O (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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
Checking if the catalog wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
WCS catalog name: wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=8049, passed=95297
Got 95297 stars (including 87119 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits.cat
util/solve_plate_with_UCAC5 got 95297 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 958 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: 0.34"
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 958 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 - 957 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits -region wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.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.ZoRPnf6um6 (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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
Checking if the catalog wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits.cat corresponding to the image wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
WCS catalog name: wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=8203, passed=97768
Got 97768 stars (including 89412 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits.cat
util/solve_plate_with_UCAC5 got 97768 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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits -region wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.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_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-00-23_20.00sec_-15.00C_LIGHT_0125.fits
Saving fully-calibrated image wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.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_Ori-03-Q1b1x1_220221_TTUQ1b1x1_16948_5AT0eIlo/wcs_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126.fits
Preparing the HTML report for the field Ori-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out125190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125219.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out126043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out125602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125929.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 125190_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125190_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:10:35.34 +04:53:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 4.841 3238893146391256064 077.64605343178 +04.89437785621 15.4355 14.9320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125192_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125192_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:11:47.19 +02:42:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125193_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125193_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:34:07.90 +05:15:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 1.174 3236677943993364096 083.53264527093 +05.25162285629 14.3828 13.7840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125195_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125195_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:15:43.53 +08:12:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125196_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125196_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 04:47:28.28 +06:58:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 3.233 3288876124651099136 071.86777737614 +06.97018704856 14.0731 13.3529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125197_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125197_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:16:59.19 +02:21:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 2.538 3234510153740723840 079.24595121756 +02.35904035299 14.4030 13.7465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125200_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125200_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:36:02.70 +02:41:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125202_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125202_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:24:41.80 +07:23:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125204_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125204_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:35:46.78 +03:18:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.139 3224308536964049408 083.94446288061 +03.30725449201 14.1068 13.5623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125205_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125205_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:39:28.05 +10:45:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 1.376 3339641023183225344 084.86680666724 +10.76501514589 13.9303 13.3906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125207_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125207_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:38:17.96 +01:41:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125209_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125209_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 04:44:51.57 +04:05:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125211_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125211_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 04:55:51.30 +09:19:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 2.969 3291301166266736128 073.96302407827 +09.32584117647 14.2853 13.7114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125212_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125212_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:24:18.93 +10:15:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125214_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125214_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:08:39.18 +08:24:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 0.945 3290070950193582080 077.16321092202 +08.41085151738 14.0414 13.5875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125217_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125217_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 04:51:58.47 +07:15:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125219_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125219_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:33:17.59 +02:28:37.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 125222_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125222_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 125224_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125224_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 04:57:22.50 +05:41:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 0.435 3239766059840274176 074.34369830624 +05.69219635871 13.7853 13.1585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125226_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125226_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:39:32.23 +10:40:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.256 3339639099037899264 084.88419227000 +10.67201986603 14.1214 13.2657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125228_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125228_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 04:53:54.60 +05:50:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125229_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125229_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:33:01.04 +01:52:42.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)
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Considering the candidate 125230_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125230_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 04:49:14.97 +08:11:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.279 3289629118317976576 072.31218462754 +08.19142104868 13.5949 13.0503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125232_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125232_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 04:55:17.80 +10:37:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125235_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125235_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 04:42:00.60 +08:04:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125238_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125238_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:10:07.17 +09:32:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 1.311 3290672859794214144 077.52974028963 +09.54066090741 12.6692 12.1266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125404_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125404_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 04:48:41.95 +09:59:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125435_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125435_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:17:00.10 +02:44:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125495_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125495_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:30:01.83 +01:46:50.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 125509_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125509_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:29:39.72 +01:56:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125579_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125579_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:29:11.12 +01:09:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125595_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125595_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:35:26.90 +01:22:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.276 3222721568024046976 083.86172873048 +01.37697616745 13.9224 13.1263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125602_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
Preparing report for the candidate 125602_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
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Considering the candidate 125603_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125603_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:21:58.84 +03:28:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125619_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
Preparing report for the candidate 125619_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
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Considering the candidate 125715_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125715_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:05:32.62 +01:26:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.768 3228786371084625792 076.38571631779 +01.44594040723 13.8317 13.2274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125718_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125718_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:24:19.62 +09:30:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 2.122 3338487394966896896 081.08127024100 +09.50931531485 13.9330 13.4432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125725_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125725_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:17:55.04 +02:58:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125763_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125763_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:32:07.82 +09:37:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125768_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125768_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 04:46:24.30 +04:16:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125875_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125875_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:33:48.94 +01:50:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125884_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125884_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:23:51.82 +01:00:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125885_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125885_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:28:18.95 +04:28:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125909_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125909_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:12:08.18 +06:49:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125911_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125911_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 04:42:45.41 +03:41:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125929_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
Preparing report for the candidate 125929_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
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Considering the candidate 125958_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125958_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:02:10.15 +02:51:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125974_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125974_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:25:20.73 +02:27:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125978_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 125978_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:20:12.80 +02:26:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 1.919 3234477271471175168 080.05381141402 +02.44362425934 14.8046 14.2849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 126043_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 126043_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 05:28:06.37 +05:14:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 1.071 3237563497531329280 082.02639665734 +05.23807313486 14.1632 13.4204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34021_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 34021_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks
**** FOUND 04:54:23.55 +07:50:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16891_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126
The candidate 16891_fd_Ori-03-Q1b1x1_2026-02-21_22-01-11_20.00sec_-14.90C_LIGHT_0126 did not pass the final checks