This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n
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 07 28.4364 2461249.9364 11.82 06:03:42.95 +33:31:12.5
177.98298 5.64835 galactic Aur Second-epoch detections are separated by 1.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.89 Julia 1 -0 1 11.6 0 0
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:03:42.95 +33:31:12.5: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:03:42.95 +33:31:12.5: 15.56 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.56 +/- 0.26
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,2461249.9364,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260728.4364 11.82CV 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 07 28.4364 2461249.9364 12.88 06:34:00.00 +42:35:31.0
172.39185 14.99844 galactic Aur Second-epoch detections are separated by 1.1" and 6.4 pix
The object was found in VSX 1" ZTF J063359.88+423531.4
Type: SR
# Max. Min./Amp. JD0 Period
12.954 r Y 1.014 r 2458312.00520 456.487300600000
The object was not found in astcheck.
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:34:00.00 +42:35:31.0: 13.80 +/- 0.04 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:34:00.00 +42:35:31.0: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
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
ZTF J063359.88+423531.4,2461249.9364,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J063359.88+423531.4 20260728.4364 12.88CV 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 07 28.4364 2461249.9364 13.00 06:00:51.57 +39:44:38.6
172.21232 8.14843 galactic Aur Second-epoch detections are separated by 0.4" and 7.1 pix
The object was found in VSX 0" CP Aur
Type: EA
# Max. Min./Amp. JD0 Period
13.220 V 14.740 V 2451274.80000 2.764500000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:00:51.57 +39:44:38.6: 14.81 +/- 0.13 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:00:51.57 +39:44:38.6: 14.77 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.09
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
CP Aur,2461249.9364,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CP Aur 20260728.4364 13.00CV 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: 2461058.73457257 18.01.2026 05:37:37.070 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
First image: 2461058.73457257 18.01.2026 05:37:37.070 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Last image: 2461249.93679729 28.07.2026 10:28:49.286 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 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
Total objects detected (at least 2 times): 22981
Objects passed selection criteria: 22815
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: 15299.5
Average stars matched: 14896.8 (97.3676 %)
Memory usage VmPeak: 249212 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jul 28 02:13:30 CDT 2026
VaST build number 1.0rc89-182-g8380f0ac
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-28)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jul 28 07:14:31 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: 2461058.73457257 18.01.2026 05:37:37.070 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
First image: 2461058.73457257 18.01.2026 05:37:37.070 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Last image: 2461249.93679729 28.07.2026 10:28:49.286 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 96
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
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: 39 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
Total objects detected (at least 2 times): 151805
Objects passed selection criteria: 151417
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: 106438
Average stars matched: 102240 (96.0566 %)
Memory usage VmPeak: 616392 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jul 28 02:13:30 CDT 2026
VaST build number 1.0rc89-182-g8380f0ac
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-28)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jul 28 07:24:10 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/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
SExtractor catalog cache: saved Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.cat to cache
SExtractor catalog cache: saved Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.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-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461249.93610152
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-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits exists and is non-empty
Saving wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits to local_wcs_cache/
'wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits' -> 'local_wcs_cache/wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits'
wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits exists and is non-empty
Saving wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits to local_wcs_cache/
'wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits' -> 'local_wcs_cache/wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits'
wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits exists and is non-empty
Saving wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits to local_wcs_cache/
'wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits' -> 'local_wcs_cache/wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits'
wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits exists and is non-empty
Saving wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits to local_wcs_cache/
'wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits' -> 'local_wcs_cache/wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits (1st reference image)
verification OK: wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.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: 06:32:42.823 +37:59:59.10 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-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits (1st new image)
verification OK: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
Image size: 945.1'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:32:32.539 +38:01:39.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:32:42.823 +37:59:59.10
Second-epoch image center 06:32:32.539 +38:01:39.10
Angular distance between the image centers 0.0437 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits (2nd new image)
verification OK: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:32:35.630 +38:01:21.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:32:42.823 +37:59:59.10
Second-epoch image center 06:32:35.630 +38:01:21.17
Angular distance between the image centers 0.0328 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 06:32:32.539 +38:01:39.10
Second-epoch second image center 06:32:35.630 +38:01:21.17
Angular distance between the image centers 0.01130 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-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits &> /tmp/tmp.425ll8QN75
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits &> /tmp/tmp.ZYD6Z8NxwV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits &> /tmp/tmp.RS9AgMsolg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits &> /tmp/tmp.4HvZJFaLka
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.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-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits and wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.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-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits and wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
Found non-empty wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits and wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
The reference image (wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits) and catalog (wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat) found
'wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat' -> 'wcsmag.cat'
Read 24697 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.6969 to 109.0146 deg, Dec +32.1595 to +43.3194 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 87.6969 to 109.0146 deg, Dec 32.1595 to 43.3194 deg
Loaded 14441 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): 10171 out of 11249 total matches.
Matched with Tycho-2 11249 out of 24697 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.927300
a=0.000000 b=1.000000 c=22.927300
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.37
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 24697 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.6969 to 109.0146 deg, Dec +32.1595 to +43.3194 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 87.6969 to 109.0146 deg, Dec 32.1595 to 43.3194 deg
Loaded 14441 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): 10171 out of 11249 total matches.
Matched with Tycho-2 11249 out of 24697 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits:
Forced-photometry filter: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits -> calib.txt_param_ref_wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits (aperture=6.2)
Read 24494 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.6949 to 109.0146 deg, Dec +32.1599 to +43.3193 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 87.6949 to 109.0146 deg, Dec 32.1599 to 43.3193 deg
Loaded 14442 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): 10145 out of 11227 total matches.
Matched with Tycho-2 11227 out of 24494 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits:
Forced-photometry filter: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits -> calib.txt_param_ref_wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
2.2 pix Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
2.5 pix fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
2.6 pix fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
2.2 pix wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
2.2 pix wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
Limiting magnitude estimates:
15.4 mag. Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
15.4 mag. Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
13.4 mag. fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
13.5 mag. fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.425ll8QN75 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.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-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits' -> 'wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.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-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
WCS-calibrated image found: wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Checking if the catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
WCS catalog name: wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=2296, bad_region=0, passed=24697
Got 24697 stars (including 22379 good ones) from the SExtractor catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
util/solve_plate_with_UCAC5 got 24697 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 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4814 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4771 matched stars entering correct_measured_positions(), 4772 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4771 matched stars entering correct_measured_positions(), 24697 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4815 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4771 matched stars entering correct_measured_positions(), 24697 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4771 matched stars entering correct_measured_positions(), 24697 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4771 stars left (next iteration limit 5248)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits N_match=4771 sigma_overall_arcsec=0.324 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.338 sigma_q3_arcsec=0.286 sigma_q4_arcsec=0.294 n_q1=1081 n_q2=1269 n_q3=1120 n_q4=1301 worst_quadrant_to_overall_ratio=1.200
The image catalog is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits -region wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ZYD6Z8NxwV (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.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-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits' -> 'wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.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-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
Checking if the catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
WCS catalog name: wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=2308, bad_region=0, passed=24494
Got 24494 stars (including 22154 good ones) from the SExtractor catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat
util/solve_plate_with_UCAC5 got 24494 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 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4812 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4766 matched stars entering correct_measured_positions(), 4768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4766 matched stars entering correct_measured_positions(), 24494 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 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4813 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4765 matched stars entering correct_measured_positions(), 24494 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4765 matched stars entering correct_measured_positions(), 24494 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4765 stars left (next iteration limit 5242)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits N_match=4765 sigma_overall_arcsec=0.366 sigma_q1_arcsec=0.445 sigma_q2_arcsec=0.367 sigma_q3_arcsec=0.320 sigma_q4_arcsec=0.332 n_q1=1060 n_q2=1286 n_q3=1120 n_q4=1299 worst_quadrant_to_overall_ratio=1.216
The image catalog is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits -region wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.RS9AgMsolg (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_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.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_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
Checking if the catalog wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
WCS catalog name: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=480, bad_region=0, passed=6279
Got 6279 stars (including 5791 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat
util/solve_plate_with_UCAC5 got 6279 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.1'
Seting catalog search parameters based on the expected field of view 945.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013126 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010501 (37.8 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 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4816 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4763 matched stars entering correct_measured_positions(), 4767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4763 matched stars entering correct_measured_positions(), 6279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4818 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4760 matched stars entering correct_measured_positions(), 6279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4760 matched stars entering correct_measured_positions(), 6279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4760 stars left (next iteration limit 5239)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4760 robust_rms=8.782 arcsec worst_quadrant_rms=11.960 arcsec
SIP_REFIT: SIP order 3 trial: matched=4760 robust_rms=0.555 arcsec worst_quadrant_rms=0.907 arcsec
SIP_REFIT: SIP order 5 trial: matched=4760 robust_rms=0.399 arcsec worst_quadrant_rms=0.508 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4760 robust_rms_before=1.726 arcsec robust_rms_before_corrected=0.434 arcsec robust_rms_after=0.399 arcsec worst_quadrant_rms_before=0.575 worst_quadrant_rms_after=0.508
verification OK: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
verification OK: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
Image size: 945.5'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:32:32.667 +38:01:37.21 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 6279 stars ###
'wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/correct_sextractor_wcs_catalog_usingxy2sky553926.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.726 -> 0.399 arcsec)
WCS_QUALITY_DIAG: file=fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits N_match=4760 sigma_overall_arcsec=0.420 sigma_q1_arcsec=0.411 sigma_q2_arcsec=0.540 sigma_q3_arcsec=0.349 sigma_q4_arcsec=0.446 n_q1=1307 n_q2=991 n_q3=1369 n_q4=1093 worst_quadrant_to_overall_ratio=1.285
The image catalog is written to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits -region wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4HvZJFaLka (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_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.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_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
Checking if the catalog wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
WCS catalog name: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=346, bad_region=0, passed=6222
Got 6222 stars (including 5869 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
util/solve_plate_with_UCAC5 got 6222 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 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 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4818 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4765 matched stars entering correct_measured_positions(), 4769 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4764 matched stars entering correct_measured_positions(), 6222 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4819 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4762 matched stars entering correct_measured_positions(), 6222 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4762 matched stars entering correct_measured_positions(), 6222 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4762 stars left (next iteration limit 5240)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4762 robust_rms=8.621 arcsec worst_quadrant_rms=12.558 arcsec
SIP_REFIT: SIP order 3 trial: matched=4762 robust_rms=0.623 arcsec worst_quadrant_rms=1.191 arcsec
SIP_REFIT: SIP order 5 trial: matched=4762 robust_rms=0.397 arcsec worst_quadrant_rms=0.499 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4762 robust_rms_before=1.668 arcsec robust_rms_before_corrected=0.425 arcsec robust_rms_after=0.397 arcsec worst_quadrant_rms_before=0.517 worst_quadrant_rms_after=0.499
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.517 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits N_match=4762 sigma_overall_arcsec=0.421 sigma_q1_arcsec=0.422 sigma_q2_arcsec=0.500 sigma_q3_arcsec=0.361 sigma_q4_arcsec=0.408 n_q1=1300 n_q2=1003 n_q3=1365 n_q4=1094 worst_quadrant_to_overall_ratio=1.188
The image catalog is written to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits -region wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits sigma_overall=0.324 worst_q_ratio=1.200
ref2=Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits sigma_overall=0.366 worst_q_ratio=1.216
new1=fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits sigma_overall=0.420 worst_q_ratio=1.285
new2=fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits sigma_overall=0.421 worst_q_ratio=1.188
reference average sigma_overall=0.345 worst_q_ratio=1.208
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224_astrometric_residuals.png (4771 matched stars from wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225_astrometric_residuals.png (4765 matched stars from wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446_astrometric_residuals.png (4760 matched stars from wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447_astrometric_residuals.png (4762 matched stars from wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits'
Saving fully-calibrated image wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits'
Preparing the HTML report for the field Aur-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12672_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 12672_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:33:49.23 +37:35:42.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07955_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 07955_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:01:07.28 +39:40:14.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Aur-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
SExtractor catalog cache: saved Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.cat to cache
SExtractor catalog cache: saved Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.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-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Creating symlink local_wcs_cache/wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits exists and is non-empty
wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits exists and is non-empty
wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits exists and is non-empty
wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits (1st reference image)
verification OK: wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.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: 06:32:42.823 +37:59:59.10 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-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits (1st new image)
verification OK: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
Image size: 945.1'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:32:32.539 +38:01:39.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:32:42.823 +37:59:59.10
Second-epoch image center 06:32:32.539 +38:01:39.10
Angular distance between the image centers 0.0437 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits (2nd new image)
verification OK: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:32:35.630 +38:01:21.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:32:42.823 +37:59:59.10
Second-epoch image center 06:32:35.630 +38:01:21.17
Angular distance between the image centers 0.0328 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 06:32:32.539 +38:01:39.10
Second-epoch second image center 06:32:35.630 +38:01:21.17
Angular distance between the image centers 0.01130 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-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits &> /tmp/tmp.Pyo5hAoYHm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits &> /tmp/tmp.yL8M7Qf7kt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits &> /tmp/tmp.IsWMqRcVtx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits &> /tmp/tmp.BvFU5sV6Q2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.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-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits and wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.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-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits and wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
Found non-empty wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits and wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
The reference image (wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits) and catalog (wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat) found
'wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat' -> 'wcsmag.cat'
Read 164929 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.6733 to 109.0146 deg, Dec +32.1595 to +43.3215 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 87.6733 to 109.0146 deg, Dec 32.1595 to 43.3215 deg
Loaded 14468 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): 8142 out of 11402 total matches.
Matched with Tycho-2 11402 out of 164929 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.799050
a=0.000000 b=1.000000 c=22.799050
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 164929 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.6733 to 109.0146 deg, Dec +32.1595 to +43.3215 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 87.6733 to 109.0146 deg, Dec 32.1595 to 43.3215 deg
Loaded 14468 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): 8142 out of 11402 total matches.
Matched with Tycho-2 11402 out of 164929 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits:
Forced-photometry filter: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits -> calib.txt_param_ref_wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits (aperture=4.8)
Read 167662 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.6656 to 109.0146 deg, Dec +32.1599 to +43.3202 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 87.6656 to 109.0146 deg, Dec 32.1599 to 43.3202 deg
Loaded 14470 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): 8100 out of 11399 total matches.
Matched with Tycho-2 11399 out of 167662 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits:
Forced-photometry filter: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits -> calib.txt_param_ref_wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 87 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
2.0 pix Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
2.5 pix fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
2.5 pix fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
2.1 pix wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
2.0 pix wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
Limiting magnitude estimates:
15.5 mag. Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
15.5 mag. Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
13.6 mag. fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
13.6 mag. fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 13.2 (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.Pyo5hAoYHm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.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-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits' -> 'wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.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-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
WCS-calibrated image found: wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Checking if the catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
WCS catalog name: wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=53, blended=19895, bad_region=2, passed=164876
Got 164876 stars (including 144720 good ones) from the SExtractor catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
util/solve_plate_with_UCAC5 got 164876 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 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4796 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4763 matched stars entering correct_measured_positions(), 4763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4763 matched stars entering correct_measured_positions(), 164876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4798 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4764 matched stars entering correct_measured_positions(), 164876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4764 matched stars entering correct_measured_positions(), 164876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4764 stars left (next iteration limit 5239)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits N_match=4764 sigma_overall_arcsec=0.322 sigma_q1_arcsec=0.353 sigma_q2_arcsec=0.333 sigma_q3_arcsec=0.293 sigma_q4_arcsec=0.306 n_q1=1113 n_q2=1253 n_q3=1148 n_q4=1250 worst_quadrant_to_overall_ratio=1.096
The image catalog is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits -region wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.yL8M7Qf7kt (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.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-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits' -> 'wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.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-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
Checking if the catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
WCS catalog name: wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=49, blended=20373, bad_region=1, passed=167613
Got 167613 stars (including 146982 good ones) from the SExtractor catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat
util/solve_plate_with_UCAC5 got 167613 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 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4798 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4770 matched stars entering correct_measured_positions(), 4770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4770 matched stars entering correct_measured_positions(), 167613 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 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4799 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4769 matched stars entering correct_measured_positions(), 167613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4769 matched stars entering correct_measured_positions(), 167613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4769 stars left (next iteration limit 5247)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits N_match=4769 sigma_overall_arcsec=0.357 sigma_q1_arcsec=0.424 sigma_q2_arcsec=0.361 sigma_q3_arcsec=0.314 sigma_q4_arcsec=0.321 n_q1=1102 n_q2=1255 n_q3=1160 n_q4=1252 worst_quadrant_to_overall_ratio=1.190
The image catalog is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits -region wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.IsWMqRcVtx (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_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.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_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
Checking if the catalog wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
WCS catalog name: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1855, bad_region=1, passed=47625
Got 47625 stars (including 45694 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat
util/solve_plate_with_UCAC5 got 47625 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.1'
Seting catalog search parameters based on the expected field of view 945.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013126 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010501 (37.8 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 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4808 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4762 matched stars entering correct_measured_positions(), 4768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4762 matched stars entering correct_measured_positions(), 47625 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4811 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4758 matched stars entering correct_measured_positions(), 47625 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4758 matched stars entering correct_measured_positions(), 47625 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4758 stars left (next iteration limit 5238)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits N_match=4758 sigma_overall_arcsec=0.424 sigma_q1_arcsec=0.410 sigma_q2_arcsec=0.557 sigma_q3_arcsec=0.357 sigma_q4_arcsec=0.449 n_q1=1307 n_q2=949 n_q3=1400 n_q4=1102 worst_quadrant_to_overall_ratio=1.313
The image catalog is written to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits -region wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BvFU5sV6Q2 (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_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.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_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
Checking if the catalog wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
WCS catalog name: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1766, bad_region=1, passed=48109
Got 48109 stars (including 46278 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
util/solve_plate_with_UCAC5 got 48109 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 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 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4815 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4770 matched stars entering correct_measured_positions(), 4776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4770 matched stars entering correct_measured_positions(), 48109 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4817 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4767 matched stars entering correct_measured_positions(), 48109 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 4767 matched stars entering correct_measured_positions(), 48109 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4767 stars left (next iteration limit 5247)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits N_match=4767 sigma_overall_arcsec=0.417 sigma_q1_arcsec=0.402 sigma_q2_arcsec=0.508 sigma_q3_arcsec=0.368 sigma_q4_arcsec=0.418 n_q1=1304 n_q2=969 n_q3=1385 n_q4=1109 worst_quadrant_to_overall_ratio=1.217
The image catalog is written to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits -region wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.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_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-27-49_20.00sec_-0.00C_LIGHTs_0446.fits
Saving fully-calibrated image wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.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_2026-07-28_CI_Aur-04-Q1b1x1_053620_TTUQ1b1x1_1318527_Q0Z5uL2n/wcs_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447.fits
Preparing the HTML report for the field Aur-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:14:05.07 +36:11:07.8: 13.30 +/- 0.03 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:09:21.77 +34:40:39.7: 13.19 +/- 0.03 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:39:41.45 +40:48:07.4: 12.76 +/- 0.02 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:18:11.84 +40:21:00.1: 13.50 +/- 0.03 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 05:57:35.25 +41:29:17.8: 13.25 +/- 0.03 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 05:53:28.16 +42:07:32.0: 13.23 +/- 0.03 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:16:51.40 +37:03:06.0: 12.39 +/- 0.01 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:14:05.07 +36:11:07.8: 13.37 +/- 0.03 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:39:41.45 +40:48:07.4: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry filter REJECTED candidate at 06:14:05.07 +36:11:07.8: ref_mag=13.33 +/- 0.02 new_mean_mag=13.1843 delta=0.15 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:09:21.77 +34:40:39.7: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter REJECTED candidate at 06:39:41.45 +40:48:07.4: ref_mag=12.76 +/- 0.01 new_mean_mag=12.8283 delta=-0.07 (need > 0.90)
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:18:11.84 +40:21:00.1: 13.42 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 06:09:21.77 +34:40:39.7: ref_mag=13.20 +/- 0.02 new_mean_mag=12.8837 delta=0.31 (need > 0.90)
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Forced photometry filter REJECTED candidate at 06:18:11.84 +40:21:00.1: ref_mag=13.46 +/- 0.02 new_mean_mag=13.0428 delta=0.42 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 05:57:35.25 +41:29:17.8: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter REJECTED candidate at 05:57:35.25 +41:29:17.8: ref_mag=13.27 +/- 0.02 new_mean_mag=13.1881 delta=0.08 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:11:54.46 +38:01:44.6: 12.30 +/- 0.01 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 05:53:28.16 +42:07:32.0: 13.21 +/- 0.03 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:16:51.40 +37:03:06.0: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter REJECTED candidate at 05:53:28.16 +42:07:32.0: ref_mag=13.22 +/- 0.02 new_mean_mag=13.0656 delta=0.15 (need > 0.90)
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry filter REJECTED candidate at 06:16:51.40 +37:03:06.0: ref_mag=12.40 +/- 0.01 new_mean_mag=12.4249 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:11:54.46 +38:01:44.6: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter REJECTED candidate at 06:11:54.46 +38:01:44.6: ref_mag=12.32 +/- 0.01 new_mean_mag=12.3694 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:03:42.95 +33:31:12.5: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:09:19.97 +33:44:03.2: 12.33 +/- 0.01 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:03:42.95 +33:31:12.5: 15.56 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.56 +/- 0.26
Forced photometry filter KEPT candidate at 06:03:42.95 +33:31:12.5: ref_mag=15.56 +/- 0.26 new_mean_mag=11.8194 delta=3.74 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:14:01.49 +33:16:04.0: 12.74 +/- 0.02 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:09:19.97 +33:44:03.2: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry filter REJECTED candidate at 06:09:19.97 +33:44:03.2: ref_mag=12.34 +/- 0.01 new_mean_mag=12.2931 delta=0.05 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:00:19.87 +38:34:37.5: 12.55 +/- 0.02 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:17:38.21 +35:07:40.7: 13.13 +/- 0.03 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:14:01.49 +33:16:04.0: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Forced photometry filter REJECTED candidate at 06:14:01.49 +33:16:04.0: ref_mag=12.72 +/- 0.02 new_mean_mag=12.5869 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:00:19.87 +38:34:37.5: 12.54 +/- 0.02 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:17:38.21 +35:07:40.7: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter REJECTED candidate at 06:00:19.87 +38:34:37.5: ref_mag=12.54 +/- 0.01 new_mean_mag=12.8197 delta=-0.28 (need > 0.90)
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter REJECTED candidate at 06:17:38.21 +35:07:40.7: ref_mag=13.10 +/- 0.02 new_mean_mag=12.8174 delta=0.28 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:48:37.93 +40:44:00.5: 12.95 +/- 0.03 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:13:18.89 +38:23:24.8: 13.49 +/- 0.03 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:19:03.17 +35:12:00.0: 13.33 +/- 0.04 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:48:37.93 +40:44:00.5: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry filter REJECTED candidate at 06:48:37.93 +40:44:00.5: ref_mag=12.95 +/- 0.02 new_mean_mag=12.8548 delta=0.09 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:19:31.16 +37:30:50.7: 13.75 +/- 0.05 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:13:18.89 +38:23:24.8: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.02
Forced photometry filter REJECTED candidate at 06:13:18.89 +38:23:24.8: ref_mag=13.54 +/- 0.02 new_mean_mag=13.1614 delta=0.37 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:19:03.17 +35:12:00.0: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter REJECTED candidate at 06:19:03.17 +35:12:00.0: ref_mag=13.32 +/- 0.02 new_mean_mag=13.1904 delta=0.13 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:19:31.16 +37:30:50.7: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter REJECTED candidate at 06:19:31.16 +37:30:50.7: ref_mag=13.73 +/- 0.03 new_mean_mag=13.4996 delta=0.23 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:34:00.00 +42:35:31.0: 13.80 +/- 0.04 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:34:00.00 +42:35:31.0: 13.80 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Forced photometry filter KEPT candidate at 06:34:00.00 +42:35:31.0: ref_mag=13.80 +/- 0.03 new_mean_mag=12.8702 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:00:51.57 +39:44:38.6: 14.81 +/- 0.13 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:00:51.57 +39:44:38.6: 14.77 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.09
Forced photometry filter KEPT candidate at 06:00:51.57 +39:44:38.6: ref_mag=14.79 +/- 0.09 new_mean_mag=12.9945 delta=1.79 (need > 0.90)
Adding exclusion_list_local.txt__out09087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49776.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190554_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190554_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190557_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190557_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:16:09.32 +39:36:06.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190560_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190560_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190561_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190561_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190562_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190562_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190564_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190564_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:14:22.86 +39:06:54.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190565_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190565_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 05:54:02.39 +37:23:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190566_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190566_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:13:16.79 +40:32:03.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190567_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190567_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:09:50.97 +37:19:41.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190568_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190568_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190570_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190570_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190573_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190573_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 05:57:20.80 +41:39:51.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190579_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190579_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:00:16.37 +42:41:12.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190586_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190586_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:32:09.88 +34:19:31.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190587_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190587_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190588_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190588_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:09:22.79 +41:44:59.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190589_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190589_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:08:27.20 +36:53:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190592_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190592_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190595_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190595_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:12:04.97 +39:00:36.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190598_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190598_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:11:57.25 +41:25:29.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190702_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190702_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:09:41.47 +37:12:00.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190798_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
Preparing report for the candidate 190798_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190812_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190812_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:09:09.90 +34:55:02.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190822_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190822_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:52:42.44 +33:55:51.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190836_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190836_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 05:59:31.65 +37:13:40.7 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190849_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190849_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:23:51.87 +39:45:38.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190858_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190858_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:57:10.66 +37:22:27.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190859_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190859_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:05:07.18 +37:56:46.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190869_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190869_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:06:07.52 +35:21:20.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190886_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190886_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:13:27.62 +37:08:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190891_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190891_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:57:29.13 +37:23:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190897_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190897_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:08:07.10 +37:57:58.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190931_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190931_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190938_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190938_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:14:05.82 +33:13:45.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190963_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 190963_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:15:09.02 +39:55:24.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191000_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191000_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 05:54:47.19 +36:14:08.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191003_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191003_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:50:07.65 +35:04:39.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191014_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191014_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:01:11.76 +41:56:59.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191036_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191036_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:16:12.93 +37:38:43.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191044_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191044_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:08:19.91 +41:02:07.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191080_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191080_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:14:35.96 +38:26:22.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191088_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191088_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:18:45.93 +38:13:35.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191112_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191112_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191119_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191119_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:38:54.45 +39:53:07.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191129_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191129_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:24:45.73 +35:16:02.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191143_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191143_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:13:49.56 +36:58:56.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191154_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191154_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:09:00.33 +34:55:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191165_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191165_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191176_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191176_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:36:45.86 +38:26:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191207_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191207_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191217_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191217_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:16:01.63 +36:11:27.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191226_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191226_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:08:27.64 +35:09:27.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191227_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191227_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:11:31.05 +38:20:30.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191228_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191228_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:17:39.52 +39:49:59.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191251_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191251_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:07:20.44 +38:04:29.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191264_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191264_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:09:33.62 +43:09:03.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191268_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191268_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:24:08.14 +39:05:27.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191269_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191269_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191283_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191283_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:50:57.06 +41:46:49.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191294_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191294_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:48:29.68 +39:33:02.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191300_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191300_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:11:41.49 +42:07:42.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191301_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191301_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191304_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191304_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:30:53.87 +39:45:25.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191330_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191330_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:17:47.46 +40:23:42.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191358_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191358_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 05:59:23.94 +40:02:36.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191372_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191372_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191373_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191373_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:17:56.84 +40:44:14.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191398_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191398_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:50:16.43 +36:25:14.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191411_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191411_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:18:11.00 +38:38:03.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191415_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191415_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:19:13.88 +37:29:56.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191431_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191431_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:25:20.61 +41:11:23.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191443_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191443_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:20:43.84 +39:19:32.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191461_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 191461_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31752_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 31752_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:15:48.74 +41:02:18.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09087_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
Preparing report for the candidate 09087_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131653_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 131653_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:02:50.61 +34:41:50.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157091_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 157091_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:52:20.07 +32:56:40.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106238_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 106238_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:06:00.39 +36:20:37.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160071_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 160071_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:38:32.74 +33:21:04.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111281_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 111281_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:28:01.80 +36:04:59.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110958_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 110958_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:15:09.54 +36:08:48.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129951_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 129951_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:18:22.87 +34:38:13.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38681_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 38681_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:07:44.05 +40:31:17.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106963_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 106963_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:16:22.16 +36:21:26.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87216_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 87216_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 06:33:49.21 +37:35:42.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51937_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447
The candidate 51937_fd_Aur-04-Q1b1x1_2026-07-28_05-28-49_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks