This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461271.7288,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260819.2288 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461271.7288,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260819.2288 11.03CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461208.90766422 17.06.2026 09:46:52.189 /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
First image: 2461208.90766422 17.06.2026 09:46:52.189 /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
Last image: 2461271.72910986 19.08.2026 05:29:45.092 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.40
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: 8 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 2655
Objects passed selection criteria: 2654
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 2450.5
Average stars matched: 2420.75 (98.786 %)
Memory usage VmPeak: 229876 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Aug 19 01:20:24 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461208.90766422 17.06.2026 09:46:52.189 /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
First image: 2461208.90766422 17.06.2026 09:46:52.189 /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
Last image: 2461271.72910986 19.08.2026 05:29:45.092 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 40
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.10
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: 12 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 18080
Objects passed selection criteria: 18049
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 16246.8
Average stars matched: 15697 (96.6162 %)
Memory usage VmPeak: 244036 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Aug 19 01:21:37 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
SExtractor catalog cache: saved PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.cat to cache
SExtractor catalog cache: saved PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.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/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.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: 2461271.72858757
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'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits exists and is non-empty
wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits exists and is non-empty
wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits exists and is non-empty
wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits (1st reference image)
verification OK: wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
Image size: 937.4'x625.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 21:54:47.944 -34:00:15.38 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits (1st new image)
verification OK: wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
Image size: 937.7'x625.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 21:54:47.374 -34:00:21.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:54:47.944 -34:00:15.38
Second-epoch image center 21:54:47.374 -34:00:21.10
Angular distance between the image centers 0.0025 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits (2nd new image)
verification OK: wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
Image size: 937.7'x625.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 21:54:47.415 -33:59:32.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:54:47.944 -34:00:15.38
Second-epoch image center 21:54:47.415 -33:59:32.46
Angular distance between the image centers 0.0121 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 21:54:47.374 -34:00:21.10
Second-epoch second image center 21:54:47.415 -33:59:32.46
Angular distance between the image centers 0.01351 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits &> /tmp/tmp.mL0QYgogUf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits &> /tmp/tmp.wU6MsRh52o
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits &> /tmp/tmp.nVUZLKos3y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits &> /tmp/tmp.I567yMvydV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
Calibrating the magnitude scale
Found non-empty wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.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_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits and wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits and wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat
Found non-empty wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits and wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat
The reference image (wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits) and catalog (wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat) found
'wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat' -> 'wcsmag.cat'
Read 3628 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 318.7196 to 338.7378 deg, Dec -39.2724 to -28.4729 deg
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
Tycho-2 catalog search boundaries: RA 318.7196 to 338.7378 deg, Dec -39.2724 to -28.4729 deg
Loaded 6219 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3002 out of 3045 total matches.
Matched with Tycho-2 3045 out of 3628 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.457900
a=0.000000 b=1.000000 c=22.457900
From vast_summary.log: estimated ref. image limiting mag.: -8.40
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.06
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.06
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 3628 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 318.7196 to 338.7378 deg, Dec -39.2724 to -28.4729 deg
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
Tycho-2 catalog search boundaries: RA 318.7196 to 338.7378 deg, Dec -39.2724 to -28.4729 deg
Loaded 6219 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3002 out of 3045 total matches.
Matched with Tycho-2 3045 out of 3628 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
Forced-photometry filter: calibrated wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits -> calib.txt_param_ref_wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits (aperture=6.2)
Read 3536 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 318.7192 to 338.6528 deg, Dec -39.2658 to -28.4732 deg
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
Tycho-2 catalog search boundaries: RA 318.7192 to 338.6528 deg, Dec -39.2658 to -28.4732 deg
Loaded 6198 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 2919 out of 2964 total matches.
Matched with Tycho-2 2964 out of 3536 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
Forced-photometry filter: calibrated wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits -> calib.txt_param_ref_wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
2.3 pix PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
2.7 pix fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
2.7 pix fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
Limiting magnitude estimates:
14.1 mag. PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
14.1 mag. PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
13.5 mag. fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
13.5 mag. fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 10.9 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.mL0QYgogUf (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_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits' -> 'wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
WCS_IMAGE_NAME=wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
WCS-calibrated image found: wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
Checking if the catalog wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat corresponding to the image wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits alredy exist and is non-empty...
Catalog wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat corresponding to the image wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
WCS catalog name: wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=236, bad_region=753, passed=3628
Got 3628 stars (including 2670 good ones) from the SExtractor catalog wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat
util/solve_plate_with_UCAC5 got 3628 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 2460 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2448 matched stars entering correct_measured_positions(), 2448 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2448 matched stars entering correct_measured_positions(), 3024 with non-zero local correction accuracy
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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 2460 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2448 matched stars entering correct_measured_positions(), 3024 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 2448 matched stars entering correct_measured_positions(), 3024 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 2448 stars left (next iteration limit 2692)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits N_match=2448 sigma_overall_arcsec=0.377 sigma_q1_arcsec=0.367 sigma_q2_arcsec=0.385 sigma_q3_arcsec=0.393 sigma_q4_arcsec=0.396 n_q1=811 n_q2=410 n_q3=825 n_q4=402 worst_quadrant_to_overall_ratio=1.050
The image catalog is written to wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits -region wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.wU6MsRh52o (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_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits' -> 'wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
WCS_IMAGE_NAME=wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
WCS-calibrated image found: wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
Checking if the catalog wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat corresponding to the image wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits alredy exist and is non-empty...
Catalog wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat corresponding to the image wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
WCS catalog name: wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=253, bad_region=766, passed=3536
Got 3536 stars (including 2558 good ones) from the SExtractor catalog wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat
util/solve_plate_with_UCAC5 got 3536 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 2364 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2352 matched stars entering correct_measured_positions(), 2353 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2352 matched stars entering correct_measured_positions(), 2913 with non-zero local correction accuracy
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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 2364 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2352 matched stars entering correct_measured_positions(), 2913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 2352 matched stars entering correct_measured_positions(), 2913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 2352 stars left (next iteration limit 2587)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits N_match=2352 sigma_overall_arcsec=0.368 sigma_q1_arcsec=0.346 sigma_q2_arcsec=0.341 sigma_q3_arcsec=0.427 sigma_q4_arcsec=0.369 n_q1=779 n_q2=404 n_q3=782 n_q4=387 worst_quadrant_to_overall_ratio=1.159
The image catalog is written to wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits -region wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nVUZLKos3y (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_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.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_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
WCS-calibrated image found: wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
Checking if the catalog wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
WCS catalog name: wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=204, bad_region=539, passed=2661
Got 2661 stars (including 1973 good ones) from the SExtractor catalog wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat
util/solve_plate_with_UCAC5 got 2661 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 1798 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1787 matched stars entering correct_measured_positions(), 1787 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1787 matched stars entering correct_measured_positions(), 2225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 1800 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1788 matched stars entering correct_measured_positions(), 2225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 1788 matched stars entering correct_measured_positions(), 2225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 1788 stars left (next iteration limit 1965)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1788 robust_rms=5.990 arcsec worst_quadrant_rms=11.912 arcsec
SIP_REFIT: SIP order 3 trial: matched=1788 robust_rms=0.690 arcsec worst_quadrant_rms=0.880 arcsec
SIP_REFIT: SIP order 5 trial: matched=1788 robust_rms=0.475 arcsec worst_quadrant_rms=0.596 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1788 robust_rms_before=1.469 arcsec robust_rms_before_corrected=0.482 arcsec robust_rms_after=0.475 arcsec worst_quadrant_rms_before=0.607 worst_quadrant_rms_after=0.596
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.607 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits N_match=1788 sigma_overall_arcsec=0.478 sigma_q1_arcsec=0.461 sigma_q2_arcsec=0.377 sigma_q3_arcsec=0.584 sigma_q4_arcsec=0.509 n_q1=646 n_q2=291 n_q3=555 n_q4=296 worst_quadrant_to_overall_ratio=1.221
The image catalog is written to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits -region wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.I567yMvydV (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_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.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_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
WCS_IMAGE_NAME=wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
WCS-calibrated image found: wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
Checking if the catalog wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat corresponding to the image wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits alredy exist and is non-empty...
Catalog wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat corresponding to the image wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
WCS catalog name: wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=201, bad_region=528, passed=2641
Got 2641 stars (including 1964 good ones) from the SExtractor catalog wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat
util/solve_plate_with_UCAC5 got 2641 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 1789 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1778 matched stars entering correct_measured_positions(), 1778 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1778 matched stars entering correct_measured_positions(), 2214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 1791 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1779 matched stars entering correct_measured_positions(), 2214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 1779 matched stars entering correct_measured_positions(), 2214 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 1779 stars left (next iteration limit 1955)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1779 robust_rms=6.007 arcsec worst_quadrant_rms=12.341 arcsec
SIP_REFIT: SIP order 3 trial: matched=1779 robust_rms=0.713 arcsec worst_quadrant_rms=0.935 arcsec
SIP_REFIT: SIP order 5 trial: matched=1779 robust_rms=0.486 arcsec worst_quadrant_rms=0.640 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1779 robust_rms_before=1.514 arcsec robust_rms_before_corrected=0.496 arcsec robust_rms_after=0.486 arcsec worst_quadrant_rms_before=0.624 worst_quadrant_rms_after=0.640
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.624 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits N_match=1779 sigma_overall_arcsec=0.492 sigma_q1_arcsec=0.488 sigma_q2_arcsec=0.360 sigma_q3_arcsec=0.662 sigma_q4_arcsec=0.498 n_q1=641 n_q2=292 n_q3=553 n_q4=293 worst_quadrant_to_overall_ratio=1.345
The image catalog is written to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits -region wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits to local_wcs_cache/
'wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits' -> 'local_wcs_cache/wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits'
Saving the final (post-refit) wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits to local_wcs_cache/
'wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits' -> 'local_wcs_cache/wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits'
Saving the final (post-refit) wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits to local_wcs_cache/
'wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits' -> 'local_wcs_cache/wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits'
Saving the final (post-refit) wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits to local_wcs_cache/
'wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits' -> 'local_wcs_cache/wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits sigma_overall=0.377 worst_q_ratio=1.050
ref2=PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits sigma_overall=0.368 worst_q_ratio=1.159
new1=fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits sigma_overall=0.478 worst_q_ratio=1.221
new2=fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits sigma_overall=0.492 worst_q_ratio=1.345
reference average sigma_overall=0.3725 worst_q_ratio=1.1045
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447_astrometric_residuals.png (2448 matched stars from wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413_astrometric_residuals.png (2352 matched stars from wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200_astrometric_residuals.png (1788 matched stars from wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201_astrometric_residuals.png (1779 matched stars from wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.45 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits'
Saving fully-calibrated image wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits'
Preparing the HTML report for the field PsA-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
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 20113_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 20113_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
**** FOUND 21:47:28.92 -36:11:47.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20114_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
Preparing report for the candidate 20114_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03232_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 03232_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
**** FOUND 21:26:44.22 -29:51:07.0 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 PsA-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
SExtractor catalog cache: saved PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.cat to cache
SExtractor catalog cache: saved PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
Creating symlink local_wcs_cache/wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
Creating symlink local_wcs_cache/wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
Creating symlink local_wcs_cache/wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
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_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits exists and is non-empty
wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits exists and is non-empty
wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits exists and is non-empty
wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits (1st reference image)
verification OK: wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
Image size: 937.4'x625.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 21:54:47.944 -34:00:15.38 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits (1st new image)
verification OK: wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
Image size: 937.7'x625.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 21:54:47.374 -34:00:21.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:54:47.944 -34:00:15.38
Second-epoch image center 21:54:47.374 -34:00:21.10
Angular distance between the image centers 0.0025 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits (2nd new image)
verification OK: wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
Image size: 937.7'x625.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 21:54:47.415 -33:59:32.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:54:47.944 -34:00:15.38
Second-epoch image center 21:54:47.415 -33:59:32.46
Angular distance between the image centers 0.0121 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 21:54:47.374 -34:00:21.10
Second-epoch second image center 21:54:47.415 -33:59:32.46
Angular distance between the image centers 0.01351 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits &> /tmp/tmp.gDLmqrtqYO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits &> /tmp/tmp.qv39Lug8KK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits &> /tmp/tmp.6zYCyHl3hI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits &> /tmp/tmp.qWMmg1f5a7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
Calibrating the magnitude scale
Found non-empty wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.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_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits and wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits and wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat
Found non-empty wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits and wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat
The reference image (wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits) and catalog (wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat) found
'wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat' -> 'wcsmag.cat'
Read 22039 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 318.7149 to 338.7378 deg, Dec -39.2736 to -28.4729 deg
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
Tycho-2 catalog search boundaries: RA 318.7149 to 338.7378 deg, Dec -39.2736 to -28.4729 deg
Loaded 6225 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4891 out of 5098 total matches.
Matched with Tycho-2 5098 out of 22039 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.306300
a=0.000000 b=1.000000 c=22.306300
From vast_summary.log: estimated ref. image limiting mag.: -8.10
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.21
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.21
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 22039 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 318.7149 to 338.7378 deg, Dec -39.2736 to -28.4729 deg
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
Tycho-2 catalog search boundaries: RA 318.7149 to 338.7378 deg, Dec -39.2736 to -28.4729 deg
Loaded 6225 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4891 out of 5098 total matches.
Matched with Tycho-2 5098 out of 22039 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
Forced-photometry filter: calibrated wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits -> calib.txt_param_ref_wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits (aperture=4.9)
Read 23094 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 318.7138 to 338.6528 deg, Dec -39.2737 to -28.4732 deg
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
Tycho-2 catalog search boundaries: RA 318.7138 to 338.6528 deg, Dec -39.2737 to -28.4732 deg
Loaded 6204 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4881 out of 5101 total matches.
Matched with Tycho-2 5101 out of 23094 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
Forced-photometry filter: calibrated wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits -> calib.txt_param_ref_wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 22 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
2.2 pix PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
2.4 pix fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
2.4 pix fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
Limiting magnitude estimates:
14.2 mag. PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
14.2 mag. PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
13.7 mag. fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
13.7 mag. fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.1 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.gDLmqrtqYO (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_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits' -> 'wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
WCS_IMAGE_NAME=wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
WCS-calibrated image found: wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
Checking if the catalog wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat corresponding to the image wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits alredy exist and is non-empty...
Catalog wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat corresponding to the image wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits
WCS catalog name: wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=646, bad_region=3158, passed=22038
Got 22038 stars (including 18353 good ones) from the SExtractor catalog wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat
util/solve_plate_with_UCAC5 got 22038 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4618 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4600 matched stars entering correct_measured_positions(), 4600 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4600 matched stars entering correct_measured_positions(), 19714 with non-zero local correction accuracy
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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4618 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4600 matched stars entering correct_measured_positions(), 19714 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4600 matched stars entering correct_measured_positions(), 19714 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4600 stars left (next iteration limit 5060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits N_match=4600 sigma_overall_arcsec=0.384 sigma_q1_arcsec=0.387 sigma_q2_arcsec=0.398 sigma_q3_arcsec=0.387 sigma_q4_arcsec=0.362 n_q1=1500 n_q2=728 n_q3=1578 n_q4=794 worst_quadrant_to_overall_ratio=1.037
The image catalog is written to wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits -region wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qv39Lug8KK (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_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits' -> 'wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
WCS_IMAGE_NAME=wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
WCS-calibrated image found: wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
Checking if the catalog wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat corresponding to the image wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits alredy exist and is non-empty...
Catalog wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat corresponding to the image wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits
WCS catalog name: wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=4, blended=748, bad_region=3453, passed=23089
Got 23089 stars (including 19032 good ones) from the SExtractor catalog wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat
util/solve_plate_with_UCAC5 got 23089 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4622 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4603 matched stars entering correct_measured_positions(), 4603 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4603 matched stars entering correct_measured_positions(), 20552 with non-zero local correction accuracy
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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4622 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4603 matched stars entering correct_measured_positions(), 20552 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4603 matched stars entering correct_measured_positions(), 20552 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4603 stars left (next iteration limit 5063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits N_match=4603 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.378 sigma_q2_arcsec=0.374 sigma_q3_arcsec=0.394 sigma_q4_arcsec=0.363 n_q1=1509 n_q2=746 n_q3=1551 n_q4=797 worst_quadrant_to_overall_ratio=1.040
The image catalog is written to wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits -region wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6zYCyHl3hI (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_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.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_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
WCS-calibrated image found: wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
Checking if the catalog wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
WCS catalog name: wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=525, bad_region=3568, passed=16943
Got 16943 stars (including 12963 good ones) from the SExtractor catalog wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat
util/solve_plate_with_UCAC5 got 16943 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4614 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4592 matched stars entering correct_measured_positions(), 4593 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4592 matched stars entering correct_measured_positions(), 14202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4615 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4592 matched stars entering correct_measured_positions(), 14202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 4592 matched stars entering correct_measured_positions(), 14202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 4592 stars left (next iteration limit 5051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4592 robust_rms=6.311 arcsec worst_quadrant_rms=11.258 arcsec
SIP_REFIT: SIP order 3 trial: matched=4592 robust_rms=0.778 arcsec worst_quadrant_rms=1.040 arcsec
SIP_REFIT: SIP order 5 trial: matched=4592 robust_rms=0.596 arcsec worst_quadrant_rms=0.794 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4592 robust_rms_before=1.558 arcsec robust_rms_before_corrected=0.594 arcsec robust_rms_after=0.596 arcsec worst_quadrant_rms_before=0.845 worst_quadrant_rms_after=0.794
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.845 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits N_match=4592 sigma_overall_arcsec=0.564 sigma_q1_arcsec=0.549 sigma_q2_arcsec=0.379 sigma_q3_arcsec=0.785 sigma_q4_arcsec=0.570 n_q1=1578 n_q2=843 n_q3=1411 n_q4=760 worst_quadrant_to_overall_ratio=1.392
The image catalog is written to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits -region wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qWMmg1f5a7 (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_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.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_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
WCS_IMAGE_NAME=wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
WCS-calibrated image found: wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
Checking if the catalog wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat corresponding to the image wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits alredy exist and is non-empty...
Catalog wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat corresponding to the image wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
WCS catalog name: wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=531, bad_region=3549, passed=17054
Got 17054 stars (including 13075 good ones) from the SExtractor catalog wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat
util/solve_plate_with_UCAC5 got 17054 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4616 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4597 matched stars entering correct_measured_positions(), 4597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4597 matched stars entering correct_measured_positions(), 14332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 4616 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4597 matched stars entering correct_measured_positions(), 14332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 4597 matched stars entering correct_measured_positions(), 14332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 4597 stars left (next iteration limit 5056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4597 robust_rms=6.388 arcsec worst_quadrant_rms=11.207 arcsec
SIP_REFIT: SIP order 3 trial: matched=4597 robust_rms=0.817 arcsec worst_quadrant_rms=1.090 arcsec
SIP_REFIT: SIP order 5 trial: matched=4597 robust_rms=0.613 arcsec worst_quadrant_rms=0.833 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4597 robust_rms_before=1.608 arcsec robust_rms_before_corrected=0.604 arcsec robust_rms_after=0.613 arcsec worst_quadrant_rms_before=0.821 worst_quadrant_rms_after=0.833
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.821 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits N_match=4597 sigma_overall_arcsec=0.572 sigma_q1_arcsec=0.566 sigma_q2_arcsec=0.423 sigma_q3_arcsec=0.771 sigma_q4_arcsec=0.541 n_q1=1574 n_q2=846 n_q3=1416 n_q4=761 worst_quadrant_to_overall_ratio=1.349
The image catalog is written to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits -region wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.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_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-28-59_20.00sec_-0.00C_LIGHT_0200.fits
Saving fully-calibrated image wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.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_2026-08-19_CI_PsA-03-Q2b1x1_010925_TTUQ2b1x1_306039_Uh3qb6nK/wcs_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201.fits
Preparing the HTML report for the field PsA-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:15:18.44 -38:07:33.0: 13.64 +/- 0.17 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:05:00.28 -38:13:21.2: 13.73 +/- 0.17 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:01:19.92 -37:44:42.1: 13.88 +/- 0.18 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 21:52:13.32 -36:42:57.5: 12.41 +/- 0.04 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:14:06.86 -37:57:58.4: 13.60 +/- 0.15 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:16:59.93 -36:53:06.8: 14.08 +/- 0.23 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:10:31.74 -37:44:45.0: 13.47 +/- 0.14 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:07:53.35 -38:11:29.4: 13.81 +/- 0.18 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:14:18.78 -37:47:40.8: 13.96 +/- 0.23 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:15:18.44 -38:07:33.0: 13.35 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.10
Forced photometry filter REJECTED candidate at 22:15:18.44 -38:07:33.0: ref_mag=13.45 +/- 0.10 new_mean_mag=13.3853 delta=0.07 (need > 0.90)
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:05:00.28 -38:13:21.2: 13.52 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.11
Forced photometry filter REJECTED candidate at 22:05:00.28 -38:13:21.2: ref_mag=13.60 +/- 0.11 new_mean_mag=13.4863 delta=0.11 (need > 0.90)
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:16:59.93 -36:53:06.8: 13.60 +/- 0.15 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:01:19.92 -37:44:42.1: 13.97 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.12
Forced photometry filter REJECTED candidate at 22:16:59.93 -36:53:06.8: ref_mag=13.74 +/- 0.12 new_mean_mag=13.6205 delta=0.11 (need > 0.90)
Forced photometry reference-image weighted average: 13.92 +/- 0.13
Forced photometry filter REJECTED candidate at 22:01:19.92 -37:44:42.1: ref_mag=13.92 +/- 0.13 new_mean_mag=13.5837 delta=0.34 (need > 0.90)
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:10:31.74 -37:44:45.0: 13.55 +/- 0.15 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:07:53.35 -38:11:29.4: 13.60 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.10
Forced photometry filter REJECTED candidate at 22:10:31.74 -37:44:45.0: ref_mag=13.51 +/- 0.10 new_mean_mag=13.2263 delta=0.28 (need > 0.90)
Forced photometry reference-image weighted average: 13.69 +/- 0.11
Forced photometry filter REJECTED candidate at 22:07:53.35 -38:11:29.4: ref_mag=13.69 +/- 0.11 new_mean_mag=13.3244 delta=0.36 (need > 0.90)
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:14:18.78 -37:47:40.8: 13.90 +/- 0.22 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.16
Forced photometry filter REJECTED candidate at 22:14:18.78 -37:47:40.8: ref_mag=13.93 +/- 0.16 new_mean_mag=13.5788 delta=0.35 (need > 0.90)
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:14:06.86 -37:57:58.4: 13.53 +/- 0.14 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 21:52:13.32 -36:42:57.5: 12.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.03
Forced photometry reference-image weighted average: 13.56 +/- 0.10
Forced photometry filter REJECTED candidate at 22:14:06.86 -37:57:58.4: ref_mag=13.56 +/- 0.10 new_mean_mag=13.4236 delta=0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:52:13.32 -36:42:57.5: ref_mag=12.46 +/- 0.03 new_mean_mag=12.6785 delta=-0.21 (need > 0.90)
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:09:12.86 -38:02:47.1: 13.95 +/- 0.21 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:16:03.36 -37:32:21.1: 13.86 +/- 0.20 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:10:27.96 -37:42:33.2: 13.71 +/- 0.17 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 21:58:05.90 -37:21:04.5: 13.98 +/- 0.19 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:12:50.85 -38:11:35.7: 13.90 +/- 0.22 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 21:45:42.22 -38:12:39.9: 13.76 +/- 0.17 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:16:03.36 -37:32:21.1: 13.91 +/- 0.20 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:09:12.86 -38:02:47.1: 13.91 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.14
Forced photometry filter REJECTED candidate at 22:09:12.86 -38:02:47.1: ref_mag=13.93 +/- 0.14 new_mean_mag=13.4785 delta=0.45 (need > 0.90)
Forced photometry reference-image weighted average: 13.89 +/- 0.14
Forced photometry filter REJECTED candidate at 22:16:03.36 -37:32:21.1: ref_mag=13.89 +/- 0.14 new_mean_mag=13.6107 delta=0.28 (need > 0.90)
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:06:59.68 -36:51:49.6: 13.84 +/- 0.17 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:10:27.96 -37:42:33.2: 14.05 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.14
Forced photometry filter REJECTED candidate at 22:10:27.96 -37:42:33.2: ref_mag=13.82 +/- 0.14 new_mean_mag=13.5681 delta=0.25 (need > 0.90)
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 21:58:05.90 -37:21:04.5: 13.84 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.12
Forced photometry filter REJECTED candidate at 21:58:05.90 -37:21:04.5: ref_mag=13.90 +/- 0.12 new_mean_mag=13.4946 delta=0.41 (need > 0.90)
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:16:20.96 -37:11:16.2: 13.77 +/- 0.18 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-17_04-46-52_20.00sec_4.90C_LIGHT_0447.fits at 22:16:34.56 -35:39:54.1: 13.80 +/- 0.17 detection
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 21:45:42.22 -38:12:39.9: 13.79 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.12
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:12:50.85 -38:11:35.7: 14.29 +/- 0.29 detection
Forced photometry filter REJECTED candidate at 21:45:42.22 -38:12:39.9: ref_mag=13.77 +/- 0.12 new_mean_mag=13.5817 delta=0.19 (need > 0.90)
Forced photometry reference-image weighted average: 14.04 +/- 0.17
Forced photometry filter REJECTED candidate at 22:12:50.85 -38:11:35.7: ref_mag=14.04 +/- 0.17 new_mean_mag=13.7971 delta=0.25 (need > 0.90)
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:06:59.68 -36:51:49.6: 13.80 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.12
Forced photometry filter REJECTED candidate at 22:06:59.68 -36:51:49.6: ref_mag=13.82 +/- 0.12 new_mean_mag=13.5725 delta=0.24 (need > 0.90)
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:16:34.56 -35:39:54.1: 14.38 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.15
Forced photometry filter REJECTED candidate at 22:16:34.56 -35:39:54.1: ref_mag=13.96 +/- 0.15 new_mean_mag=13.6415 delta=0.32 (need > 0.90)
Forced photometry on wcs_PsA-03-Q2b1x1_2026-06-18_04-43-41_20.00sec_4.90C_LIGHT_0413.fits at 22:16:20.96 -37:11:16.2: 13.57 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.12
Forced photometry filter REJECTED candidate at 22:16:20.96 -37:11:16.2: ref_mag=13.65 +/- 0.12 new_mean_mag=13.5613 delta=0.09 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 4s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31874_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31874_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31883_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
Preparing report for the candidate 31883_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31908_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31908_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31909_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31909_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31910_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31910_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31912_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31912_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31920_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31920_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31922_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31922_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31927_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31927_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31928_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31928_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31934_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31934_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31937_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31937_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31942_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31942_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31947_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31947_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31949_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31949_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31963_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31963_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31973_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31973_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31978_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31978_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31990_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 31990_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05170_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 05170_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
**** FOUND 21:47:28.91 -36:11:47.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17921_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 17921_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks
**** FOUND 21:26:44.22 -29:51:06.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16610_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201
The candidate 16610_fd_PsA-03-Q2b1x1_2026-08-19_00-29-45_20.00sec_-0.00C_LIGHT_0201 did not pass the final checks