This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 10 09.1892 2461322.6892 12.07 05:05:09.42 +26:06:06.8
177.34556 -9.02518 galactic Tau Second-epoch detections are separated by 0.3" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.49 Pales 0 0 0 12.2 0 0
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:05:09.42 +26:06:06.8: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:05:09.42 +26:06:06.8: 16.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 09.1892* 05 05 09.42 +26 06 06.8 12.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461322.6892,12.07,0.05,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 20261009.1892 12.07CV 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
Mean magnitude and position on the discovery images:
2026 10 09.1892 2461322.6892 13.60 05:12:49.38 +30:05:36.7
175.09230 -5.31129 galactic Aur Second-epoch detections are separated by 0.8" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.359 Georgia -0 -0 0 13.9 0 0
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:12:49.38 +30:05:36.7: 15.91 +/- 0.27 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:12:49.38 +30:05:36.7: 16.17 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.91 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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,2461322.6892,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.1892 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
First image: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Last image: 2461322.68945728 09.10.2026 04:32:39.109 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 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): 13762
Objects passed selection criteria: 13677
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 9021
Average stars matched: 8476 (93.9585 %)
Memory usage VmPeak: 239316 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Oct 9 04:57:08 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
First image: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Last image: 2461322.68945728 09.10.2026 04:32:39.109 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 55
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -6.99
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: 29 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): 108096
Objects passed selection criteria: 107838
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 76449.5
Average stars matched: 71435.8 (93.4417 %)
Memory usage VmPeak: 569164 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Oct 9 04:58:22 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
SExtractor catalog cache: saved Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat to cache
SExtractor catalog cache: saved Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461322.68888899
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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits exists and is non-empty
wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits exists and is non-empty
wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits exists and is non-empty
wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (1st reference image)
verification OK: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:00:01.042 +29:59:39.82 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits (1st new image)
verification OK: wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
Image size: 941.3'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 05:00:00.491 +29:59:54.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:00:01.042 +29:59:39.82
Second-epoch image center 05:00:00.491 +29:59:54.28
Angular distance between the image centers 0.0045 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits (2nd new image)
verification OK: wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
Image size: 941.2'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 05:00:03.390 +30:00:33.37 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:00:01.042 +29:59:39.82
Second-epoch image center 05:00:03.390 +30:00:33.37
Angular distance between the image centers 0.0171 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:00:00.491 +29:59:54.28
Second-epoch second image center 05:00:03.390 +30:00:33.37
Angular distance between the image centers 0.01508 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits &> /tmp/tmp.U1Je3yyejM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits &> /tmp/tmp.Rck7RYYNnU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits &> /tmp/tmp.MzA63cQ30q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits &> /tmp/tmp.0SxWpkHiBB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
Found non-empty wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
The reference image (wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits) and catalog (wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat) found
'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat' -> 'wcsmag.cat'
Read 16295 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5633 to 84.6655 deg, Dec +24.3644 to +35.2863 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 65.5633 to 84.6655 deg, Dec 24.3644 to 35.2863 deg
Loaded 8426 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): 6039 out of 6740 total matches.
Matched with Tycho-2 6740 out of 16295 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.981000
a=0.000000 b=1.000000 c=22.981000
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.65
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.65
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 16295 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5633 to 84.6655 deg, Dec +24.3644 to +35.2863 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 65.5633 to 84.6655 deg, Dec 24.3644 to 35.2863 deg
Loaded 8426 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): 6039 out of 6740 total matches.
Matched with Tycho-2 6740 out of 16295 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Forced-photometry filter: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -> calib.txt_param_ref_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (aperture=5.9)
Read 16349 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5633 to 84.6688 deg, Dec +24.3644 to +35.2864 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 65.5633 to 84.6688 deg, Dec 24.3644 to 35.2864 deg
Loaded 8429 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): 6042 out of 6743 total matches.
Matched with Tycho-2 6743 out of 16349 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Forced-photometry filter: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -> calib.txt_param_ref_wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
2.3 pix fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
2.4 pix fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
Limiting magnitude estimates:
15.7 mag. Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
15.7 mag. Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
14.5 mag. fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
14.5 mag. fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.4 (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.U1Je3yyejM (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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=1498, bad_region=2648, passed=16295
Got 16295 stars (including 12280 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
util/solve_plate_with_UCAC5 got 16295 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4843 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4803 matched stars entering correct_measured_positions(), 4802 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4803 matched stars entering correct_measured_positions(), 14059 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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4843 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4802 matched stars entering correct_measured_positions(), 14059 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4802 matched stars entering correct_measured_positions(), 14059 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4802 stars left (next iteration limit 5283)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits N_match=4802 sigma_overall_arcsec=0.392 sigma_q1_arcsec=0.417 sigma_q2_arcsec=0.299 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.271 n_q1=2427 n_q2=541 n_q3=1322 n_q4=512 worst_quadrant_to_overall_ratio=1.065
The image catalog is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -region wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Rck7RYYNnU (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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=1486, bad_region=2654, passed=16349
Got 16349 stars (including 12341 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat
util/solve_plate_with_UCAC5 got 16349 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4842 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4799 matched stars entering correct_measured_positions(), 4799 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4799 matched stars entering correct_measured_positions(), 14119 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4842 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4797 matched stars entering correct_measured_positions(), 14119 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4797 matched stars entering correct_measured_positions(), 14119 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4797 stars left (next iteration limit 5278)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits N_match=4797 sigma_overall_arcsec=0.377 sigma_q1_arcsec=0.406 sigma_q2_arcsec=0.283 sigma_q3_arcsec=0.331 sigma_q4_arcsec=0.279 n_q1=2431 n_q2=544 n_q3=1318 n_q4=504 worst_quadrant_to_overall_ratio=1.079
The image catalog is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -region wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.MzA63cQ30q (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_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.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_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.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=332, bad_region=2119, passed=6566
Got 6566 stars (including 4220 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat
util/solve_plate_with_UCAC5 got 6566 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4077 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4042 matched stars entering correct_measured_positions(), 4042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4042 matched stars entering correct_measured_positions(), 4918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4075 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4040 matched stars entering correct_measured_positions(), 4918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 4040 matched stars entering correct_measured_positions(), 4918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 4040 stars left (next iteration limit 4446)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4040 robust_rms=6.714 arcsec worst_region_rms=11.413 arcsec outer_annulus_rms=11.413 arcsec
SIP_REFIT: SIP order 3 trial: matched=4040 robust_rms=0.759 arcsec worst_region_rms=0.989 arcsec outer_annulus_rms=0.989 arcsec
SIP_REFIT: SIP order 5 trial: matched=4040 robust_rms=0.595 arcsec worst_region_rms=0.874 arcsec outer_annulus_rms=0.874 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4040 robust_rms_before=1.699 arcsec robust_rms_before_corrected=0.569 arcsec robust_rms_after=0.595 arcsec worst_region_rms_before=0.928 worst_region_rms_after=0.874 outer_annulus_rms_before=1.426 outer_annulus_rms_after=0.874
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.928 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits worst_region_rms_kept=0.928 arcsec robust_rms_kept=0.569 arcsec matched=4040
WCS_QUALITY_DIAG: file=fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits N_match=4040 sigma_overall_arcsec=0.571 sigma_q1_arcsec=0.578 sigma_q2_arcsec=0.555 sigma_q3_arcsec=0.700 sigma_q4_arcsec=0.520 n_q1=804 n_q2=710 n_q3=1277 n_q4=1249 worst_quadrant_to_overall_ratio=1.226
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits -region wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.0SxWpkHiBB (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_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.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=335, bad_region=2124, passed=6648
Got 6648 stars (including 4291 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat
util/solve_plate_with_UCAC5 got 6648 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4145 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4111 matched stars entering correct_measured_positions(), 4112 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4111 matched stars entering correct_measured_positions(), 5001 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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4144 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4111 matched stars entering correct_measured_positions(), 5001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 4111 matched stars entering correct_measured_positions(), 5001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 4111 stars left (next iteration limit 4522)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4111 robust_rms=6.691 arcsec worst_region_rms=12.219 arcsec outer_annulus_rms=12.219 arcsec
SIP_REFIT: SIP order 3 trial: matched=4111 robust_rms=0.719 arcsec worst_region_rms=1.008 arcsec outer_annulus_rms=1.008 arcsec
SIP_REFIT: SIP order 5 trial: matched=4111 robust_rms=0.565 arcsec worst_region_rms=0.840 arcsec outer_annulus_rms=0.840 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4111 robust_rms_before=1.687 arcsec robust_rms_before_corrected=0.554 arcsec robust_rms_after=0.565 arcsec worst_region_rms_before=0.874 worst_region_rms_after=0.840 outer_annulus_rms_before=1.435 outer_annulus_rms_after=0.840
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.874 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits worst_region_rms_kept=0.874 arcsec robust_rms_kept=0.554 arcsec matched=4111
WCS_QUALITY_DIAG: file=fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits N_match=4111 sigma_overall_arcsec=0.563 sigma_q1_arcsec=0.551 sigma_q2_arcsec=0.563 sigma_q3_arcsec=0.677 sigma_q4_arcsec=0.526 n_q1=817 n_q2=714 n_q3=1297 n_q4=1283 worst_quadrant_to_overall_ratio=1.201
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits -region wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits to local_wcs_cache/
'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'local_wcs_cache/wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
Saving the final (post-refit) wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits to local_wcs_cache/
'wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'local_wcs_cache/wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
Saving the final (post-refit) wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits'
Saving the final (post-refit) wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits sigma_overall=0.392 worst_q_ratio=1.065
ref2=Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits sigma_overall=0.377 worst_q_ratio=1.079
new1=fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits sigma_overall=0.571 worst_q_ratio=1.226
new2=fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits sigma_overall=0.563 worst_q_ratio=1.201
reference average sigma_overall=0.3845 worst_q_ratio=1.072
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362_astrometric_residuals.png (4802 matched stars from wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363_astrometric_residuals.png (4797 matched stars from wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230_astrometric_residuals.png (4040 matched stars from wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.52 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231_astrometric_residuals.png (4111 matched stars from wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits'
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits'
Preparing the HTML report for the field Aur-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Aur-05-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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
SExtractor catalog cache: saved Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat to cache
SExtractor catalog cache: saved Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Creating symlink local_wcs_cache/wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
Checking 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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits exists and is non-empty
wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits exists and is non-empty
wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits exists and is non-empty
wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (1st reference image)
verification OK: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:00:01.042 +29:59:39.82 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits (1st new image)
verification OK: wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
Image size: 941.3'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 05:00:00.491 +29:59:54.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:00:01.042 +29:59:39.82
Second-epoch image center 05:00:00.491 +29:59:54.28
Angular distance between the image centers 0.0045 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits (2nd new image)
verification OK: wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
Image size: 941.2'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 05:00:03.390 +30:00:33.37 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:00:01.042 +29:59:39.82
Second-epoch image center 05:00:03.390 +30:00:33.37
Angular distance between the image centers 0.0171 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:00:00.491 +29:59:54.28
Second-epoch second image center 05:00:03.390 +30:00:33.37
Angular distance between the image centers 0.01508 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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits &> /tmp/tmp.INcBwecUyp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits &> /tmp/tmp.lMkxeKFXA6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits &> /tmp/tmp.eLsntMgVlF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits &> /tmp/tmp.HIl3awIIfu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
Found non-empty wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
The reference image (wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits) and catalog (wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat) found
'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat' -> 'wcsmag.cat'
Read 129003 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5559 to 84.6888 deg, Dec +24.3225 to +35.3000 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 65.5559 to 84.6888 deg, Dec 24.3225 to 35.3000 deg
Loaded 8484 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): 4942 out of 6871 total matches.
Matched with Tycho-2 6871 out of 129003 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.831850
a=0.000000 b=1.000000 c=22.831850
From vast_summary.log: estimated ref. image limiting mag.: -6.99
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.84
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.84
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 129003 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5559 to 84.6888 deg, Dec +24.3225 to +35.3000 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 65.5559 to 84.6888 deg, Dec 24.3225 to 35.3000 deg
Loaded 8484 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): 4942 out of 6871 total matches.
Matched with Tycho-2 6871 out of 129003 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Forced-photometry filter: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -> calib.txt_param_ref_wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (aperture=4.4)
Read 129055 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5633 to 84.6902 deg, Dec +24.3185 to +35.2955 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 65.5633 to 84.6902 deg, Dec 24.3185 to 35.2955 deg
Loaded 8479 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): 4936 out of 6879 total matches.
Matched with Tycho-2 6879 out of 129055 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Forced-photometry filter: calibrated wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -> calib.txt_param_ref_wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 49 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.8 pix Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
2.1 pix fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
2.2 pix fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
Limiting magnitude estimates:
15.8 mag. Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
15.8 mag. Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
14.7 mag. fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
14.7 mag. fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.0 (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.INcBwecUyp (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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=22, blended=14027, bad_region=17069, passed=128981
Got 128981 stars (including 98831 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
util/solve_plate_with_UCAC5 got 128981 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 4838 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4808 matched stars entering correct_measured_positions(), 4808 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4808 matched stars entering correct_measured_positions(), 115119 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 4838 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4807 matched stars entering correct_measured_positions(), 115119 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4807 matched stars entering correct_measured_positions(), 115119 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4807 stars left (next iteration limit 5288)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits N_match=4807 sigma_overall_arcsec=0.358 sigma_q1_arcsec=0.384 sigma_q2_arcsec=0.291 sigma_q3_arcsec=0.339 sigma_q4_arcsec=0.241 n_q1=2304 n_q2=552 n_q3=1394 n_q4=557 worst_quadrant_to_overall_ratio=1.071
The image catalog is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -region wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.lMkxeKFXA6 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat corresponding to the image wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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=22, blended=13827, bad_region=17078, passed=129033
Got 129033 stars (including 99032 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat
util/solve_plate_with_UCAC5 got 129033 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 4836 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4804 matched stars entering correct_measured_positions(), 4804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4804 matched stars entering correct_measured_positions(), 115182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 4836 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4804 matched stars entering correct_measured_positions(), 115182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4804 matched stars entering correct_measured_positions(), 115182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4804 stars left (next iteration limit 5284)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits N_match=4804 sigma_overall_arcsec=0.362 sigma_q1_arcsec=0.385 sigma_q2_arcsec=0.289 sigma_q3_arcsec=0.344 sigma_q4_arcsec=0.252 n_q1=2299 n_q2=560 n_q3=1389 n_q4=556 worst_quadrant_to_overall_ratio=1.064
The image catalog is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -region wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.eLsntMgVlF (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_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.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_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.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=11, blended=2655, bad_region=13198, passed=55160
Got 55160 stars (including 39985 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat
util/solve_plate_with_UCAC5 got 55160 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4821 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 4783 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 45656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4819 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4784 matched stars entering correct_measured_positions(), 45656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4784 matched stars entering correct_measured_positions(), 45656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 4784 stars left (next iteration limit 5261)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.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=4784 robust_rms=6.542 arcsec worst_region_rms=13.666 arcsec outer_annulus_rms=13.666 arcsec
SIP_REFIT: SIP order 3 trial: matched=4784 robust_rms=0.759 arcsec worst_region_rms=1.001 arcsec outer_annulus_rms=1.001 arcsec
SIP_REFIT: SIP order 5 trial: matched=4784 robust_rms=0.598 arcsec worst_region_rms=0.860 arcsec outer_annulus_rms=0.860 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4784 robust_rms_before=1.726 arcsec robust_rms_before_corrected=0.547 arcsec robust_rms_after=0.598 arcsec worst_region_rms_before=0.902 worst_region_rms_after=0.860 outer_annulus_rms_before=1.407 outer_annulus_rms_after=0.860
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.902 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits worst_region_rms_kept=0.902 arcsec robust_rms_kept=0.547 arcsec matched=4784
WCS_QUALITY_DIAG: file=fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits N_match=4784 sigma_overall_arcsec=0.553 sigma_q1_arcsec=0.594 sigma_q2_arcsec=0.529 sigma_q3_arcsec=0.670 sigma_q4_arcsec=0.507 n_q1=983 n_q2=894 n_q3=1407 n_q4=1500 worst_quadrant_to_overall_ratio=1.212
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits -region wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.HIl3awIIfu (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_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.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=5, blended=2667, bad_region=13302, passed=55269
Got 55269 stars (including 40000 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat
util/solve_plate_with_UCAC5 got 55269 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4823 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4786 matched stars entering correct_measured_positions(), 4786 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4786 matched stars entering correct_measured_positions(), 45732 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4821 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4786 matched stars entering correct_measured_positions(), 45732 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4786 matched stars entering correct_measured_positions(), 45732 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 4786 stars left (next iteration limit 5264)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.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=4786 robust_rms=6.465 arcsec worst_region_rms=14.074 arcsec outer_annulus_rms=14.074 arcsec
SIP_REFIT: SIP order 3 trial: matched=4786 robust_rms=0.714 arcsec worst_region_rms=1.038 arcsec outer_annulus_rms=1.038 arcsec
SIP_REFIT: SIP order 5 trial: matched=4786 robust_rms=0.578 arcsec worst_region_rms=0.859 arcsec outer_annulus_rms=0.859 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4786 robust_rms_before=1.717 arcsec robust_rms_before_corrected=0.540 arcsec robust_rms_after=0.578 arcsec worst_region_rms_before=0.892 worst_region_rms_after=0.859 outer_annulus_rms_before=1.450 outer_annulus_rms_after=0.859
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.892 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits worst_region_rms_kept=0.892 arcsec robust_rms_kept=0.540 arcsec matched=4786
WCS_QUALITY_DIAG: file=fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits N_match=4786 sigma_overall_arcsec=0.551 sigma_q1_arcsec=0.538 sigma_q2_arcsec=0.503 sigma_q3_arcsec=0.690 sigma_q4_arcsec=0.513 n_q1=990 n_q2=888 n_q3=1401 n_q4=1507 worst_quadrant_to_overall_ratio=1.253
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits -region wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.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_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-31-50_20.00sec_-0.00C_LIGHT_0230.fits
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Aur-05-Q2b1x1_045357_TTUQ2b1x1_3220212_bm9ECkhi/wcs_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231.fits
Preparing the HTML report for the field Aur-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:43:52.76 +26:43:12.5: 13.74 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:52:18.10 +31:47:11.5: 12.38 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:41:09.84 +28:51:29.8: 13.92 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:07:57.59 +29:14:13.3: 14.15 +/- 0.07 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:50:57.65 +29:41:27.0: 12.87 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:47:09.79 +33:15:09.9: 12.54 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:16:21.64 +32:50:24.2: 12.40 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:05:09.42 +26:06:06.8: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:43:52.76 +26:43:12.5: 13.81 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry filter REJECTED candidate at 04:43:52.76 +26:43:12.5: ref_mag=13.77 +/- 0.03 new_mean_mag=13.7841 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:16:21.64 +32:50:24.2: 12.41 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:52:18.10 +31:47:11.5: 12.40 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:07:57.59 +29:14:13.3: 14.30 +/- 0.08 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:41:09.84 +28:51:29.8: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:47:09.79 +33:15:09.9: 12.54 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 05:16:21.64 +32:50:24.2: ref_mag=12.40 +/- 0.01 new_mean_mag=12.5995 delta=-0.20 (need > 0.90)
Forced photometry reference-image weighted average: 14.22 +/- 0.05
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:50:57.65 +29:41:27.0: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry filter REJECTED candidate at 05:07:57.59 +29:14:13.3: ref_mag=14.22 +/- 0.05 new_mean_mag=14.1775 delta=0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:52:18.10 +31:47:11.5: ref_mag=12.40 +/- 0.01 new_mean_mag=12.6751 delta=-0.28 (need > 0.90)
Forced photometry reference-image weighted average: 13.94 +/- 0.03
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter REJECTED candidate at 04:41:09.84 +28:51:29.8: ref_mag=13.94 +/- 0.03 new_mean_mag=14.0037 delta=-0.06 (need > 0.90)
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry filter REJECTED candidate at 04:47:09.79 +33:15:09.9: ref_mag=12.54 +/- 0.01 new_mean_mag=12.7448 delta=-0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:50:57.65 +29:41:27.0: ref_mag=12.86 +/- 0.01 new_mean_mag=13.2245 delta=-0.36 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:05:09.42 +26:06:06.8: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:17:10.95 +32:04:56.6: 13.23 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:17:10.58 +27:23:38.8: 13.14 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:59:17.36 +32:33:43.1: 13.74 +/- 0.05 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:17:10.95 +32:04:56.6: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter REJECTED candidate at 05:17:10.95 +32:04:56.6: ref_mag=13.25 +/- 0.02 new_mean_mag=13.1396 delta=0.11 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:17:10.58 +27:23:38.8: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter REJECTED candidate at 05:17:10.58 +27:23:38.8: ref_mag=13.10 +/- 0.02 new_mean_mag=13.1614 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:14:17.49 +33:04:32.6: 13.75 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:59:17.36 +32:33:43.1: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry filter REJECTED candidate at 04:59:17.36 +32:33:43.1: ref_mag=13.75 +/- 0.03 new_mean_mag=13.5089 delta=0.24 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:04:43.87 +30:15:53.6: 14.34 +/- 0.06 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:14:17.49 +33:04:32.6: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Forced photometry filter REJECTED candidate at 05:14:17.49 +33:04:32.6: ref_mag=13.76 +/- 0.03 new_mean_mag=13.7011 delta=0.06 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:12:49.38 +30:05:36.7: 15.91 +/- 0.27 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:04:43.87 +30:15:53.6: 14.36 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.04
Forced photometry filter REJECTED candidate at 05:04:43.87 +30:15:53.6: ref_mag=14.35 +/- 0.04 new_mean_mag=14.2185 delta=0.13 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:12:49.38 +30:05:36.7: 16.17 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.91 +/- 0.27
Forced photometry filter KEPT candidate at 05:12:49.38 +30:05:36.7: ref_mag=15.91 +/- 0.27 new_mean_mag=13.5967 delta=2.31 (need > 0.90)
Adding exclusion_list_local.txt__out151143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74507.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 41s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 149650_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 149650_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 04:58:10.32 +28:15:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149651_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 149651_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
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Considering the candidate 149662_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 149662_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
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Considering the candidate 149676_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 149676_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
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Considering the candidate 149686_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 149686_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
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Considering the candidate 149693_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 149693_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 04:57:39.91 +29:07:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149694_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 149694_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
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Considering the candidate 149695_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 149695_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
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Considering the candidate 149696_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 149696_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
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Considering the candidate 150864_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 150864_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 04:56:57.81 +33:05:59.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 151143_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
Preparing report for the candidate 151143_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
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Considering the candidate 151188_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 151188_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:18:18.09 +33:47:32.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151459_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 151459_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 04:56:56.98 +33:06:50.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 151485_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 151485_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:15:29.74 +32:42:36.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 152128_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 152128_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:14:46.52 +31:23:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152132_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 152132_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 04:51:21.96 +28:31:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152304_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 152304_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:05:45.92 +26:25:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152722_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 152722_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:18:28.45 +33:11:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153537_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 153537_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:01:54.45 +28:18:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153821_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 153821_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
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Considering the candidate 153827_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 153827_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 04:48:17.71 +29:45:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153850_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 153850_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
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Considering the candidate 153860_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 153860_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 04:41:13.47 +28:37:09.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 153974_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 153974_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:09:45.68 +28:00:27.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 154021_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 154021_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:09:49.68 +29:48:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154023_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 154023_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 04:48:18.84 +29:47:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154180_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 154180_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:04:49.96 +29:58:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154473_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 154473_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:19:18.29 +33:59:47.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 154649_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 154649_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
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Considering the candidate 154896_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 154896_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:19:27.51 +34:00:25.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 155001_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 155001_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:17:17.95 +33:11:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155205_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 155205_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:19:17.35 +31:00:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155275_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 155275_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:12:52.68 +32:19:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155546_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 155546_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 04:49:22.09 +29:33:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155602_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 155602_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
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Considering the candidate 155800_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 155800_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:15:58.62 +32:57:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155871_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 155871_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 04:59:24.14 +31:04:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156181_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 156181_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 04:49:41.67 +28:20:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156244_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 156244_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 04:59:38.18 +31:15:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156372_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 156372_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:19:43.69 +26:10:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157446_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 157446_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:05:53.05 +31:14:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157480_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 157480_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
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Considering the candidate 143958_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 143958_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:10:32.21 +32:10:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105568_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 105568_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:15:47.42 +26:45:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128243_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 128243_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 04:58:51.38 +28:31:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74507_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
Preparing report for the candidate 74507_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
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Considering the candidate 121345_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 121345_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 05:03:15.43 +28:42:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85504_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 85504_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks
**** FOUND 04:47:48.55 +29:25:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62858_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231
The candidate 62858_fd_Aur-05-Q2b1x1_2026-10-08_23-32-39_20.00sec_0.00C_LIGHT_0231 did not pass the final checks