This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw
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 08.1923 2461321.6923 12.13 05:04:45.44 +26:05:18.5
177.30268 -9.10542 galactic Tau Second-epoch detections are separated by 0.5" and 9.0 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 12.3 0 0
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:04:45.44 +26:05:18.5: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:04:45.44 +26:05:18.5: 16.23 +/- 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 08.1923* 05 04 45.44 +26 05 18.5 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,2461321.6923,12.13,0.05,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 20261008.1923 12.13CV 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 08.1923 2461321.6923 13.56 05:12:34.29 +30:01:33.7
175.11548 -5.39487 galactic Aur Second-epoch detections are separated by 1.4" and 8.6 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 -1 1 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 05:12:34.29 +30:01:33.7: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:12:34.29 +30:01:33.7: 15.93 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.93 +/- 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,2461321.6923,13.56,0.05,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 20261008.1923 13.56CV 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: 2461321.69257586 08.10.2026 04:37:08.554 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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: 5 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): 13805
Objects passed selection criteria: 13718
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: 9079.75
Average stars matched: 8527.25 (93.915 %)
Memory usage VmPeak: 239320 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 Thu Oct 8 04:15:48 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: 2461321.69257586 08.10.2026 04:37:08.554 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 58
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: 25 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): 108673
Objects passed selection criteria: 108418
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: 77459.2
Average stars matched: 72276.8 (93.3094 %)
Memory usage VmPeak: 569168 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 Thu Oct 8 04:16:59 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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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: 2461321.69194267
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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits exists and is non-empty
wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits (1st new image)
verification OK: wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.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: 05:00:00.760 +30:00:04.20 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 05:00:00.760 +30:00:04.20
Angular distance between the image centers 0.0068 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits (2nd new image)
verification OK: wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
Image size: 941.1'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: 04:59:58.250 +29:59:24.78 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 04:59:58.250 +29:59:24.78
Angular distance between the image centers 0.0109 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 05:00:00.760 +30:00:04.20
Second-epoch second image center 04:59:58.250 +29:59:24.78
Angular distance between the image centers 0.01421 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.IPJ7zi5w1A
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.qMMPIkDvds
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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits &> /tmp/tmp.38EKmK3wPj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits &> /tmp/tmp.OoHaeIkH14
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
2.4 pix fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
14.5 mag. fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.5 (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.IPJ7zi5w1A (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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/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.qMMPIkDvds (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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/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.38EKmK3wPj (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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.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=351, bad_region=2139, passed=6728
Got 6728 stars (including 4355 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits.wcscat
util/solve_plate_with_UCAC5 got 6728 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 4203 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4167 matched stars entering correct_measured_positions(), 4167 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4167 matched stars entering correct_measured_positions(), 5061 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 4202 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4166 matched stars entering correct_measured_positions(), 5061 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 4166 matched stars entering correct_measured_positions(), 5062 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 4166 stars left (next iteration limit 4583)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4166 robust_rms=6.636 arcsec worst_region_rms=11.235 arcsec outer_annulus_rms=11.235 arcsec
SIP_REFIT: SIP order 3 trial: matched=4166 robust_rms=0.655 arcsec worst_region_rms=0.970 arcsec outer_annulus_rms=0.970 arcsec
SIP_REFIT: SIP order 5 trial: matched=4166 robust_rms=0.531 arcsec worst_region_rms=0.772 arcsec outer_annulus_rms=0.772 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4166 robust_rms_before=1.490 arcsec robust_rms_before_corrected=0.531 arcsec robust_rms_after=0.531 arcsec worst_region_rms_before=0.830 worst_region_rms_after=0.772 outer_annulus_rms_before=1.316 outer_annulus_rms_after=0.772
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.830 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits worst_region_rms_kept=0.830 arcsec robust_rms_kept=0.531 arcsec matched=4166
WCS_QUALITY_DIAG: file=fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits N_match=4166 sigma_overall_arcsec=0.542 sigma_q1_arcsec=0.540 sigma_q2_arcsec=0.532 sigma_q3_arcsec=0.642 sigma_q4_arcsec=0.508 n_q1=816 n_q2=726 n_q3=1348 n_q4=1276 worst_quadrant_to_overall_ratio=1.185
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits -region wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.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.OoHaeIkH14 (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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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=348, bad_region=2189, passed=6810
Got 6810 stars (including 4383 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat
util/solve_plate_with_UCAC5 got 6810 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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 4231 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4194 matched stars entering correct_measured_positions(), 4194 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4194 matched stars entering correct_measured_positions(), 5112 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 4229 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4195 matched stars entering correct_measured_positions(), 5112 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 4195 matched stars entering correct_measured_positions(), 5112 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 4195 stars left (next iteration limit 4613)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4195 robust_rms=6.584 arcsec worst_region_rms=11.206 arcsec outer_annulus_rms=11.206 arcsec
SIP_REFIT: SIP order 3 trial: matched=4195 robust_rms=0.645 arcsec worst_region_rms=0.945 arcsec outer_annulus_rms=0.945 arcsec
SIP_REFIT: SIP order 5 trial: matched=4195 robust_rms=0.534 arcsec worst_region_rms=0.771 arcsec outer_annulus_rms=0.771 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4195 robust_rms_before=1.447 arcsec robust_rms_before_corrected=0.545 arcsec robust_rms_after=0.534 arcsec worst_region_rms_before=0.818 worst_region_rms_after=0.771 outer_annulus_rms_before=1.308 outer_annulus_rms_after=0.771
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.818 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits worst_region_rms_kept=0.818 arcsec robust_rms_kept=0.545 arcsec matched=4195
WCS_QUALITY_DIAG: file=fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits N_match=4195 sigma_overall_arcsec=0.536 sigma_q1_arcsec=0.515 sigma_q2_arcsec=0.548 sigma_q3_arcsec=0.651 sigma_q4_arcsec=0.487 n_q1=841 n_q2=735 n_q3=1338 n_q4=1281 worst_quadrant_to_overall_ratio=1.213
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits -region wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits'
Saving the final (post-refit) wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits sigma_overall=0.542 worst_q_ratio=1.185
new2=fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits sigma_overall=0.536 worst_q_ratio=1.213
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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216_astrometric_residuals.png (4166 matched stars from wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.50 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217_astrometric_residuals.png (4195 matched stars from wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits'
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits exists and is non-empty
wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits (1st new image)
verification OK: wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.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: 05:00:00.760 +30:00:04.20 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 05:00:00.760 +30:00:04.20
Angular distance between the image centers 0.0068 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits (2nd new image)
verification OK: wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
Image size: 941.1'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: 04:59:58.250 +29:59:24.78 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 04:59:58.250 +29:59:24.78
Angular distance between the image centers 0.0109 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 05:00:00.760 +30:00:04.20
Second-epoch second image center 04:59:58.250 +29:59:24.78
Angular distance between the image centers 0.01421 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.Xi1YIGj7aC
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.JJqqrB44tx
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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits &> /tmp/tmp.eWG6Yo0f0o
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits &> /tmp/tmp.qkzLdrac8O
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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 54 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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
2.1 pix fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
14.7 mag. fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Xi1YIGj7aC (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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/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.JJqqrB44tx (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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/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.eWG6Yo0f0o (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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.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=14, blended=2912, bad_region=13431, passed=57418
Got 57418 stars (including 41802 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits.wcscat
util/solve_plate_with_UCAC5 got 57418 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 4824 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 4782 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 47759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 4824 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4780 matched stars entering correct_measured_positions(), 47759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 4780 matched stars entering correct_measured_positions(), 47759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4780 stars left (next iteration limit 5260)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.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=4780 robust_rms=6.432 arcsec worst_region_rms=13.013 arcsec outer_annulus_rms=13.013 arcsec
SIP_REFIT: SIP order 3 trial: matched=4780 robust_rms=0.649 arcsec worst_region_rms=0.986 arcsec outer_annulus_rms=0.986 arcsec
SIP_REFIT: SIP order 5 trial: matched=4780 robust_rms=0.536 arcsec worst_region_rms=0.817 arcsec outer_annulus_rms=0.817 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4780 robust_rms_before=1.521 arcsec robust_rms_before_corrected=0.521 arcsec robust_rms_after=0.536 arcsec worst_region_rms_before=0.850 worst_region_rms_after=0.817 outer_annulus_rms_before=1.291 outer_annulus_rms_after=0.817
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.850 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits worst_region_rms_kept=0.850 arcsec robust_rms_kept=0.521 arcsec matched=4780
WCS_QUALITY_DIAG: file=fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits N_match=4780 sigma_overall_arcsec=0.532 sigma_q1_arcsec=0.503 sigma_q2_arcsec=0.538 sigma_q3_arcsec=0.621 sigma_q4_arcsec=0.505 n_q1=998 n_q2=876 n_q3=1430 n_q4=1476 worst_quadrant_to_overall_ratio=1.168
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits -region wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.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.qkzLdrac8O (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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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=12, blended=2892, bad_region=13586, passed=57601
Got 57601 stars (including 41835 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat
util/solve_plate_with_UCAC5 got 57601 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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: 4784 matched stars entering correct_measured_positions(), 4784 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4784 matched stars entering correct_measured_positions(), 47880 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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
Accuracy estimation diagnostic: 4784 matched stars entering correct_measured_positions(), 47880 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 4784 matched stars entering correct_measured_positions(), 47880 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4784 stars left (next iteration limit 5262)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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=6.390 arcsec worst_region_rms=13.396 arcsec outer_annulus_rms=13.396 arcsec
SIP_REFIT: SIP order 3 trial: matched=4784 robust_rms=0.637 arcsec worst_region_rms=0.954 arcsec outer_annulus_rms=0.954 arcsec
SIP_REFIT: SIP order 5 trial: matched=4784 robust_rms=0.538 arcsec worst_region_rms=0.798 arcsec outer_annulus_rms=0.798 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4784 robust_rms_before=1.469 arcsec robust_rms_before_corrected=0.522 arcsec robust_rms_after=0.538 arcsec worst_region_rms_before=0.825 worst_region_rms_after=0.798 outer_annulus_rms_before=1.305 outer_annulus_rms_after=0.798
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.825 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits worst_region_rms_kept=0.825 arcsec robust_rms_kept=0.522 arcsec matched=4784
WCS_QUALITY_DIAG: file=fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits N_match=4784 sigma_overall_arcsec=0.519 sigma_q1_arcsec=0.508 sigma_q2_arcsec=0.532 sigma_q3_arcsec=0.660 sigma_q4_arcsec=0.483 n_q1=989 n_q2=879 n_q3=1421 n_q4=1495 worst_quadrant_to_overall_ratio=1.271
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits -region wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-36-13_20.00sec_-0.00C_LIGHT_0216.fits
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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_2026-10-08_CI_Aur-05-Q2b1x1_041304_TTUQ2b1x1_38396_xmEa1tbw/wcs_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217.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 05:01:28.61 +31:02:36.9: 14.25 +/- 0.05 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:03:07.74 +33:55:23.5: 13.95 +/- 0.05 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:01:57.08 +29:41:40.4: 14.24 +/- 0.06 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:06:35.07 +32:59:01.8: 13.41 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:14:19.54 +33:19:39.2: 13.85 +/- 0.05 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:40:40.77 +32:42:25.4: 13.99 +/- 0.05 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:56:57.83 +33:05:59.0: 11.96 +/- 0.01 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:18:38.83 +33:39:16.2: 12.81 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:01:28.61 +31:02:36.9: 14.28 +/- 0.05 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:40:40.77 +32:42:25.4: 14.01 +/- 0.05 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:01:57.08 +29:41:40.4: 14.23 +/- 0.06 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:14:19.54 +33:19:39.2: 13.85 +/- 0.05 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:03:07.74 +33:55:23.5: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.04
Forced photometry filter REJECTED candidate at 05:01:28.61 +31:02:36.9: ref_mag=14.26 +/- 0.04 new_mean_mag=14.2857 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 14.00 +/- 0.03
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:06:35.07 +32:59:01.8: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.04
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Forced photometry filter REJECTED candidate at 04:40:40.77 +32:42:25.4: ref_mag=14.00 +/- 0.03 new_mean_mag=14.1495 delta=-0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:01:57.08 +29:41:40.4: ref_mag=14.23 +/- 0.04 new_mean_mag=14.2481 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:14:19.54 +33:19:39.2: ref_mag=13.85 +/- 0.03 new_mean_mag=13.7945 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.98 +/- 0.03
Forced photometry filter REJECTED candidate at 05:03:07.74 +33:55:23.5: ref_mag=13.98 +/- 0.03 new_mean_mag=14.1101 delta=-0.13 (need > 0.90)
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Forced photometry filter REJECTED candidate at 05:06:35.07 +32:59:01.8: ref_mag=13.41 +/- 0.02 new_mean_mag=13.5177 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:04:45.44 +26:05:18.5: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:56:57.83 +33:05:59.0: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Forced photometry filter REJECTED candidate at 04:56:57.83 +33:05:59.0: ref_mag=11.96 +/- 0.01 new_mean_mag=11.8737 delta=0.08 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:18:38.83 +33:39:16.2: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter REJECTED candidate at 05:18:38.83 +33:39:16.2: ref_mag=12.78 +/- 0.01 new_mean_mag=12.8681 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:14:54.13 +31:02:58.0: 12.75 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:04:45.44 +26:05:18.5: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:14:37.79 +32:20:21.4: 13.27 +/- 0.03 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:14:54.13 +31:02:58.0: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry filter REJECTED candidate at 05:14:54.13 +31:02:58.0: ref_mag=12.74 +/- 0.01 new_mean_mag=12.6443 delta=0.09 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:17:10.61 +27:23:40.1: 13.17 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:14:37.79 +32:20:21.4: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter REJECTED candidate at 05:14:37.79 +32:20:21.4: ref_mag=13.28 +/- 0.02 new_mean_mag=13.1882 delta=0.09 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:58:17.11 +30:17:39.4: 13.71 +/- 0.04 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:17:10.61 +27:23:40.1: 13.09 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter REJECTED candidate at 05:17:10.61 +27:23:40.1: ref_mag=13.13 +/- 0.02 new_mean_mag=13.1803 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:08:04.76 +28:22:42.7: 14.01 +/- 0.05 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:58:17.11 +30:17:39.4: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Forced photometry filter REJECTED candidate at 04:58:17.11 +30:17:39.4: ref_mag=13.69 +/- 0.03 new_mean_mag=13.6609 delta=0.03 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:17:05.16 +32:13:49.1: 13.91 +/- 0.05 detection
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:08:04.76 +28:22:42.7: 14.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.04
Forced photometry filter REJECTED candidate at 05:08:04.76 +28:22:42.7: ref_mag=14.08 +/- 0.04 new_mean_mag=13.8665 delta=0.21 (need > 0.90)
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:12:34.29 +30:01:33.7: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q2b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:17:05.16 +32:13:49.1: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.03
Forced photometry filter REJECTED candidate at 05:17:05.16 +32:13:49.1: ref_mag=13.93 +/- 0.03 new_mean_mag=13.9357 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 05:12:34.29 +30:01:33.7: 15.93 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.93 +/- 0.27
Forced photometry filter KEPT candidate at 05:12:34.29 +30:01:33.7: ref_mag=15.93 +/- 0.27 new_mean_mag=13.5564 delta=2.37 (need > 0.90)
Adding exclusion_list_local.txt__out151271.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75479.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 149645_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 149645_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:00:28.78 +28:48:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149654_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 149654_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 149655_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 149655_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 149656_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 149656_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:17:36.61 +32:03:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149661_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 149661_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 149662_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 149662_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 04:58:10.51 +28:15:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149664_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 149664_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 149668_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 149668_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 149674_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 149674_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:03:36.99 +33:23:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149685_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 149685_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 149695_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 149695_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 149697_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 149697_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 04:42:31.57 +31:29:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150824_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 150824_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 151182_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 151182_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:18:18.05 +33:47:32.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151271_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
Preparing report for the candidate 151271_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
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Considering the candidate 151424_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 151424_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:15:29.76 +32:42:36.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 152135_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 152135_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 152211_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 152211_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:14:46.53 +31:23:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152325_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 152325_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 04:51:21.98 +28:31:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152701_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 152701_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:05:45.93 +26:25:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153013_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 153013_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:18:28.50 +33:11:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153407_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 153407_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:17:19.58 +33:12:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153666_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 153666_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 153971_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 153971_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:17:17.87 +33:11:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154006_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 154006_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 04:48:18.80 +29:47:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154032_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 154032_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 154397_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 154397_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:09:49.73 +29:48:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154446_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 154446_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:04:49.95 +29:58:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154455_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 154455_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 04:48:17.72 +29:45:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154597_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 154597_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:19:43.63 +26:10:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154817_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 154817_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:19:18.23 +33:59:47.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 154865_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 154865_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:15:58.50 +32:57:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155046_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 155046_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:19:17.26 +31:00:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155442_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 155442_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:12:52.64 +32:19:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155622_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 155622_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:19:27.54 +34:00:25.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 155674_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 155674_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 155699_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 155699_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 04:59:24.14 +31:04:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155737_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 155737_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:04:38.96 +32:11:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155958_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 155958_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 04:59:38.17 +31:15:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156055_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 156055_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:10:31.71 +30:49:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157006_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 157006_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:05:52.91 +31:14:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157368_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 157368_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 157408_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 157408_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:07:47.84 +30:15:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157617_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 157617_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 04:49:41.68 +28:20:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157704_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 157704_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
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Considering the candidate 158005_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 158005_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:04:21.09 +29:22:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75479_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
Preparing report for the candidate 75479_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
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Considering the candidate 143958_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 143958_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:10:32.19 +32:10:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105568_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 105568_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:15:47.35 +26:45:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128243_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 128243_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 04:58:51.42 +28:31:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121914_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 121914_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:09:38.46 +28:39:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121345_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 121345_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:03:15.46 +28:42:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70065_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 70065_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks
**** FOUND 05:07:49.50 +30:24:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62858_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217
The candidate 62858_fd_Aur-05-Q2b1x1_2026-10-07_23-37-08_20.00sec_-0.00C_LIGHT_0217 did not pass the final checks