This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW
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 28.3926 2461249.8926 8.88 05:27:07.45 +34:08:59.3
173.48645 -0.51105 galactic Aur Second-epoch detections are separated by 0.3" and 8.8 pix
The object was found in VSX 0" S Aur
Type: SR
# Max. Min./Amp. JD0 Period
8.200 V 13.300 V 2442000.00000 590.100000000000 C4-5,4-5(N3)
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:27:07.45 +34:08:59.3: 10.12 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:27:07.45 +34:08:59.3: 9.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.83 +/- 0.00
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
S Aur,2461249.8926,8.88,0.05,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
S Aur 20260728.3926 8.88CV 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 28.3926 2461249.8926 8.64 06:01:07.16 +39:40:14.0
172.30169 8.15701 galactic Aur Second-epoch detections are separated by 0.7" and 9.1 pix
The object was found in VSX 1" AZ Aur
Type: M
# Max. Min./Amp. JD0 Period
8.100 V 14.000 V 2454467.00000 411.900000000000 C7,1e-C8,2-3(N0e)
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:07.16 +39:40:14.0: 10.12 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:07.16 +39:40:14.0: 9.99 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.04 +/- 0.00
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
AZ Aur,2461249.8926,8.64,0.05,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
AZ Aur 20260728.3926 8.64CV 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 28.3926 2461249.8926 11.88 04:50:00.90 +39:55:58.0
164.42859 -2.99178 galactic Per Second-epoch detections are separated by 0.4" and 8.2 pix
The object was found in VSX 1" NSVS J0450006+395559
Type: M
# Max. Min./Amp. JD0 Period
10.700 R1 Y 2.092 R1 730.000000000000 N
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:50:00.90 +39:55:58.0: 13.47 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:50:00.90 +39:55:58.0: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 28.3926* 04 50 00.90 +39 55 58.0 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0450006+395559,2461249.8926,11.88,0.05,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
NSVS J0450006+395559 20260728.3926 11.88CV 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 28.3926 2461249.8926 11.86 05:58:41.92 +40:42:08.8
171.16303 8.24843 galactic Aur Second-epoch detections are separated by 1.0" and 9.0 pix
The object was found in VSX 1" ASASSN-V J055842.01+404209.1
Type: L
# Max. Min./Amp. JD0 Period
13.260 V 13.620 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:58:41.92 +40:42:08.8: 12.96 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:58:41.92 +40:42:08.8: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
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
ASASSN-V J055842.01+404209.1,2461249.8926,11.86,0.05,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
ASASSN-V J055842.01+404209.1 20260728.3926 11.86CV 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 28.3926 2461249.8926 11.82 05:46:50.05 +37:10:02.6
173.08636 4.48517 galactic Aur Second-epoch detections are separated by 1.0" and 9.0 pix
The object was found in VSX 0" V0344 Aur
Type: SR:
# Max. Min./Amp. JD0 Period
16.700 B 18.200 B 375.000000000000 : C(N)
ATTENTION: measured mag 11.82 is 4.9 mag brighter than the VSX record maximum brightness 16.70 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:46:50.05 +37:10:02.6: 12.72 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:46:50.05 +37:10:02.6: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
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
V0344 Aur,2461249.8926,11.82,0.05,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
V0344 Aur 20260728.3926 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461249.89297750 28.07.2026 09:25:43.256 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 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): 24116
Objects passed selection criteria: 23954
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 16077.8
Average stars matched: 15275.5 (95.0102 %)
Memory usage VmPeak: 249960 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 05:14:58 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: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461249.89297750 28.07.2026 09:25:43.256 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 93
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
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: 50 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): 180720
Objects passed selection criteria: 180155
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: 124468
Average stars matched: 116030 (93.2209 %)
Memory usage VmPeak: 649020 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 05:29:53 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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
SExtractor catalog cache: saved Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.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: 2461249.89221619
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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
Saving wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits to local_wcs_cache/
'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits'
wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits exists and is non-empty
Saving wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits to local_wcs_cache/
'wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'local_wcs_cache/wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits'
wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits exists and is non-empty
Saving wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits to local_wcs_cache/
'wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits' -> 'local_wcs_cache/wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits'
wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits exists and is non-empty
Saving wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits to local_wcs_cache/
'wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits' -> 'local_wcs_cache/wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (1st reference image)
verification OK: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:17.024 +37:59:58.79 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-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits (1st new image)
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
Image size: 944.8'x626.8' 15.7(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: 05:27:07.509 +38:00:47.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:27:17.024 +37:59:58.79
Second-epoch image center 05:27:07.509 +38:00:47.43
Angular distance between the image centers 0.0340 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits (2nd new image)
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
Image size: 944.7'x626.8' 15.7(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: 05:27:10.125 +38:01:28.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:27:17.024 +37:59:58.79
Second-epoch image center 05:27:10.125 +38:01:28.28
Angular distance between the image centers 0.0336 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:27:07.509 +38:00:47.43
Second-epoch second image center 05:27:10.125 +38:01:28.28
Angular distance between the image centers 0.01423 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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.7V7eCElgBs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits &> /tmp/tmp.fDI84h8QG2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits &> /tmp/tmp.uzoL5bG37U
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits &> /tmp/tmp.C503HjMfq7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Found non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
The reference image (wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat) found
'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat' -> 'wcsmag.cat'
Read 27843 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8766 to 92.1250 deg, Dec +31.9889 to +43.3926 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 70.8766 to 92.1250 deg, Dec 31.9889 to 43.3926 deg
Loaded 16031 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): 11098 out of 12445 total matches.
Matched with Tycho-2 12445 out of 27843 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.926900
a=0.000000 b=1.000000 c=22.926900
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 27843 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8766 to 92.1250 deg, Dec +31.9889 to +43.3926 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 70.8766 to 92.1250 deg, Dec 31.9889 to 43.3926 deg
Loaded 16031 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): 11098 out of 12445 total matches.
Matched with Tycho-2 12445 out of 27843 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits:
Forced-photometry filter: calibrated wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (aperture=6.2)
Read 27116 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3508 to 92.6935 deg, Dec +32.1410 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 71.3508 to 92.6935 deg, Dec 32.1410 to 43.3194 deg
Loaded 16021 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): 10961 out of 12446 total matches.
Matched with Tycho-2 12446 out of 27116 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits:
Forced-photometry filter: calibrated wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -> calib.txt_param_ref_wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
2.1 pix Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
2.6 pix fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
2.6 pix fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
2.2 pix wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
2.1 pix wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Limiting magnitude estimates:
15.2 mag. Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
15.2 mag. Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
13.0 mag. fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
13.0 mag. fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 10.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.7V7eCElgBs (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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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=2982, bad_region=0, passed=27843
Got 27843 stars (including 24835 good ones) from the SExtractor catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
util/solve_plate_with_UCAC5 got 27843 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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 4825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 27843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 27843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 27843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4821 stars left (next iteration limit 5306)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits N_match=4821 sigma_overall_arcsec=0.361 sigma_q1_arcsec=0.452 sigma_q2_arcsec=0.366 sigma_q3_arcsec=0.353 sigma_q4_arcsec=0.300 n_q1=919 n_q2=1327 n_q3=1362 n_q4=1213 worst_quadrant_to_overall_ratio=1.253
The image catalog is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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.fDI84h8QG2 (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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Checking if the catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS catalog name: wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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=3147, bad_region=0, passed=27116
Got 27116 stars (including 23937 good ones) from the SExtractor catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
util/solve_plate_with_UCAC5 got 27116 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 4826 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 27116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 4888 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 27116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 27116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4823 stars left (next iteration limit 5306)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits N_match=4823 sigma_overall_arcsec=0.526 sigma_q1_arcsec=0.633 sigma_q2_arcsec=0.501 sigma_q3_arcsec=0.467 sigma_q4_arcsec=0.475 n_q1=1116 n_q2=1449 n_q3=1299 n_q4=959 worst_quadrant_to_overall_ratio=1.203
The image catalog is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -region wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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.uzoL5bG37U (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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
Checking if the catalog wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
WCS catalog name: wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.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=287, bad_region=0, passed=4907
Got 4907 stars (including 4614 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat
util/solve_plate_with_UCAC5 got 4907 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.8'
Seting catalog search parameters based on the expected field of view 944.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013122 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010498 (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 4519 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4450 matched stars entering correct_measured_positions(), 4454 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4450 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4516 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4449 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 4449 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 4449 stars left (next iteration limit 4895)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4449 robust_rms=8.054 arcsec worst_quadrant_rms=11.621 arcsec
SIP_REFIT: SIP order 3 trial: matched=4449 robust_rms=0.545 arcsec worst_quadrant_rms=0.976 arcsec
SIP_REFIT: SIP order 5 trial: matched=4449 robust_rms=0.464 arcsec worst_quadrant_rms=0.601 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4449 robust_rms_before=1.515 arcsec robust_rms_before_corrected=0.471 arcsec robust_rms_after=0.464 arcsec worst_quadrant_rms_before=0.572 worst_quadrant_rms_after=0.601
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.572 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits N_match=4449 sigma_overall_arcsec=0.464 sigma_q1_arcsec=0.461 sigma_q2_arcsec=0.582 sigma_q3_arcsec=0.387 sigma_q4_arcsec=0.449 n_q1=1077 n_q2=1141 n_q3=1379 n_q4=852 worst_quadrant_to_overall_ratio=1.253
The image catalog is written to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits -region wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.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.C503HjMfq7 (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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
Checking if the catalog wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
WCS catalog name: wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.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=283, bad_region=0, passed=4801
Got 4801 stars (including 4512 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits.wcscat
util/solve_plate_with_UCAC5 got 4801 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.7'
Seting catalog search parameters based on the expected field of view 944.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013121 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010497 (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 4422 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4352 matched stars entering correct_measured_positions(), 4355 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4352 matched stars entering correct_measured_positions(), 4801 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4421 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4352 matched stars entering correct_measured_positions(), 4801 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 4352 matched stars entering correct_measured_positions(), 4801 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 4352 stars left (next iteration limit 4787)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4352 robust_rms=8.345 arcsec worst_quadrant_rms=11.207 arcsec
SIP_REFIT: SIP order 3 trial: matched=4352 robust_rms=0.589 arcsec worst_quadrant_rms=0.944 arcsec
SIP_REFIT: SIP order 5 trial: matched=4352 robust_rms=0.453 arcsec worst_quadrant_rms=0.578 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4352 robust_rms_before=1.423 arcsec robust_rms_before_corrected=0.486 arcsec robust_rms_after=0.453 arcsec worst_quadrant_rms_before=0.593 worst_quadrant_rms_after=0.578
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.593 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits N_match=4352 sigma_overall_arcsec=0.467 sigma_q1_arcsec=0.470 sigma_q2_arcsec=0.561 sigma_q3_arcsec=0.393 sigma_q4_arcsec=0.492 n_q1=1043 n_q2=1130 n_q3=1336 n_q4=843 worst_quadrant_to_overall_ratio=1.201
The image catalog is written to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits -region wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits sigma_overall=0.361 worst_q_ratio=1.253
ref2=Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits sigma_overall=0.526 worst_q_ratio=1.203
new1=fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits sigma_overall=0.464 worst_q_ratio=1.253
new2=fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits sigma_overall=0.467 worst_q_ratio=1.201
reference average sigma_overall=0.4435 worst_q_ratio=1.228
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049_astrometric_residuals.png (4821 matched stars from wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054_astrometric_residuals.png (4823 matched stars from wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.47 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416_astrometric_residuals.png (4449 matched stars from wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417_astrometric_residuals.png (4352 matched stars from wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits'
Saving fully-calibrated image wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits'
Preparing the HTML report for the field Aur-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:07.16 +39:40:14.0: 10.12 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:27:07.45 +34:08:59.3: 10.12 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:07.16 +39:40:14.0: 9.99 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:27:07.45 +34:08:59.3: 9.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.04 +/- 0.00
Forced photometry filter KEPT candidate at 06:01:07.16 +39:40:14.0: ref_mag=10.04 +/- 0.00 new_mean_mag=8.6453 delta=1.40 (need > 0.90)
Forced photometry reference-image weighted average: 9.83 +/- 0.00
Forced photometry filter KEPT candidate at 05:27:07.45 +34:08:59.3: ref_mag=9.83 +/- 0.00 new_mean_mag=8.8773 delta=0.95 (need > 0.90)
Adding exclusion_list_local.txt__out03860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16474.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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 33157_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 33157_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:26:54.57 +36:54:11.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33166_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 33166_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:57:03.20 +33:08:20.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33173_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 33173_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:07:56.89 +37:48:57.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03860_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
Preparing report for the candidate 03860_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16474_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
Preparing report for the candidate 16474_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06908_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 06908_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:18:19.01 +35:14:59.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Aur-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:27:07.45 +34:08:59.3
06:01:07.16 +39:40:14.0
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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
SExtractor catalog cache: saved Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Creating symlink local_wcs_cache/wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits exists and is non-empty
wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits exists and is non-empty
wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (1st reference image)
verification OK: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:17.024 +37:59:58.79 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-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits (1st new image)
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
Image size: 944.8'x626.8' 15.7(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: 05:27:07.509 +38:00:47.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:27:17.024 +37:59:58.79
Second-epoch image center 05:27:07.509 +38:00:47.43
Angular distance between the image centers 0.0340 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits (2nd new image)
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
Image size: 944.7'x626.8' 15.7(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: 05:27:10.125 +38:01:28.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:27:17.024 +37:59:58.79
Second-epoch image center 05:27:10.125 +38:01:28.28
Angular distance between the image centers 0.0336 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:27:07.509 +38:00:47.43
Second-epoch second image center 05:27:10.125 +38:01:28.28
Angular distance between the image centers 0.01423 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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.p0xCi5hKOZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits &> /tmp/tmp.9kIwyRiW2k
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits &> /tmp/tmp.IumREe5n55
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits &> /tmp/tmp.6HvBj01pwh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Found non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
The reference image (wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat) found
'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat' -> 'wcsmag.cat'
Read 202315 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8154 to 92.1472 deg, Dec +31.9889 to +43.3931 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 70.8154 to 92.1472 deg, Dec 31.9889 to 43.3931 deg
Loaded 16059 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): 8333 out of 12787 total matches.
Matched with Tycho-2 12787 out of 202315 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.787200
a=0.000000 b=1.000000 c=22.787200
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 202315 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8154 to 92.1472 deg, Dec +31.9889 to +43.3931 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 70.8154 to 92.1472 deg, Dec 31.9889 to 43.3931 deg
Loaded 16059 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): 8333 out of 12787 total matches.
Matched with Tycho-2 12787 out of 202315 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits:
Forced-photometry filter: calibrated wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (aperture=4.7)
Read 212259 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3349 to 92.7190 deg, Dec +32.1410 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 71.3349 to 92.7190 deg, Dec 32.1410 to 43.3202 deg
Loaded 16044 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): 8107 out of 12844 total matches.
Matched with Tycho-2 12844 out of 212259 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits:
Forced-photometry filter: calibrated wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -> calib.txt_param_ref_wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 84 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
1.9 pix Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
2.5 pix fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
2.5 pix fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
2.1 pix wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
1.9 pix wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Limiting magnitude estimates:
15.4 mag. Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
15.4 mag. Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
13.2 mag. fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
13.2 mag. fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.8 (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.p0xCi5hKOZ (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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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=55, blended=30655, bad_region=1, passed=202260
Got 202260 stars (including 171302 good ones) from the SExtractor catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
util/solve_plate_with_UCAC5 got 202260 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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 4826 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 202260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4822 matched stars entering correct_measured_positions(), 202260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4822 matched stars entering correct_measured_positions(), 202260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4822 stars left (next iteration limit 5306)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits N_match=4822 sigma_overall_arcsec=0.362 sigma_q1_arcsec=0.468 sigma_q2_arcsec=0.358 sigma_q3_arcsec=0.352 sigma_q4_arcsec=0.312 n_q1=927 n_q2=1360 n_q3=1305 n_q4=1230 worst_quadrant_to_overall_ratio=1.291
The image catalog is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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.9kIwyRiW2k (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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Checking if the catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS catalog name: wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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=55, blended=32150, bad_region=8, passed=212204
Got 212204 stars (including 179717 good ones) from the SExtractor catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
util/solve_plate_with_UCAC5 got 212204 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 4823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 212204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 212204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 212204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4820 stars left (next iteration limit 5303)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits N_match=4820 sigma_overall_arcsec=0.500 sigma_q1_arcsec=0.573 sigma_q2_arcsec=0.486 sigma_q3_arcsec=0.460 sigma_q4_arcsec=0.450 n_q1=1097 n_q2=1411 n_q3=1324 n_q4=988 worst_quadrant_to_overall_ratio=1.146
The image catalog is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -region wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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.IumREe5n55 (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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
Checking if the catalog wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
WCS catalog name: wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.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=4, blended=1554, bad_region=1, passed=43520
Got 43520 stars (including 41908 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat
util/solve_plate_with_UCAC5 got 43520 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.8'
Seting catalog search parameters based on the expected field of view 944.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013122 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010498 (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 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 4816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 43520 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 43520 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 43520 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4813 stars left (next iteration limit 5295)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits N_match=4813 sigma_overall_arcsec=0.451 sigma_q1_arcsec=0.442 sigma_q2_arcsec=0.547 sigma_q3_arcsec=0.365 sigma_q4_arcsec=0.469 n_q1=1143 n_q2=1160 n_q3=1554 n_q4=956 worst_quadrant_to_overall_ratio=1.214
The image catalog is written to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits -region wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.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.6HvBj01pwh (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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
Checking if the catalog wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
WCS catalog name: wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.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=1, blended=1481, bad_region=1, passed=42471
Got 42471 stars (including 40926 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits.wcscat
util/solve_plate_with_UCAC5 got 42471 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.7'
Seting catalog search parameters based on the expected field of view 944.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013121 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010497 (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 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 4816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 42471 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 42471 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 42471 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4813 stars left (next iteration limit 5294)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits N_match=4813 sigma_overall_arcsec=0.467 sigma_q1_arcsec=0.462 sigma_q2_arcsec=0.556 sigma_q3_arcsec=0.396 sigma_q4_arcsec=0.495 n_q1=1148 n_q2=1162 n_q3=1560 n_q4=943 worst_quadrant_to_overall_ratio=1.190
The image catalog is written to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits -region wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.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-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-24-37_20.00sec_-0.00C_LIGHTs_0416.fits
Saving fully-calibrated image wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.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-03-Q1b1x1_051027_TTUQ1b1x1_322103_wMUzO1sW/wcs_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417.fits
Preparing the HTML report for the field Aur-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:17:08.13 +40:00:38.7: 11.70 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:34:00.13 +41:59:16.6: 12.04 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:34:00.13 +41:59:16.6: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry filter REJECTED candidate at 05:34:00.13 +41:59:16.6: ref_mag=12.11 +/- 0.01 new_mean_mag=11.9871 delta=0.12 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:17:08.13 +40:00:38.7: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Forced photometry filter REJECTED candidate at 05:17:08.13 +40:00:38.7: ref_mag=11.72 +/- 0.01 new_mean_mag=12.1574 delta=-0.44 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:24:50.00 +37:22:47.4: 12.65 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:14:49.26 +39:31:05.3: 12.64 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:57:29.12 +38:18:48.9: 13.18 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:15:04.83 +35:21:45.7: 13.12 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:24:50.00 +37:22:47.4: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter REJECTED candidate at 05:24:50.00 +37:22:47.4: ref_mag=12.61 +/- 0.01 new_mean_mag=12.4160 delta=0.19 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:09:59.40 +40:08:08.0: 12.88 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:57:29.12 +38:18:48.9: 13.13 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:14:49.26 +39:31:05.3: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter REJECTED candidate at 04:57:29.12 +38:18:48.9: ref_mag=13.16 +/- 0.02 new_mean_mag=12.8800 delta=0.28 (need > 0.90)
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Forced photometry filter REJECTED candidate at 05:14:49.26 +39:31:05.3: ref_mag=12.68 +/- 0.02 new_mean_mag=12.5906 delta=0.09 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:15:04.83 +35:21:45.7: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Forced photometry filter REJECTED candidate at 05:15:04.83 +35:21:45.7: ref_mag=13.09 +/- 0.03 new_mean_mag=12.9060 delta=0.18 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:09:59.40 +40:08:08.0: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry filter REJECTED candidate at 05:09:59.40 +40:08:08.0: ref_mag=12.88 +/- 0.02 new_mean_mag=12.7291 delta=0.15 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:50:00.90 +39:55:58.0: 13.47 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:50:00.90 +39:55:58.0: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 04:50:00.90 +39:55:58.0: ref_mag=13.21 +/- 0.02 new_mean_mag=11.8827 delta=1.32 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:58:41.92 +40:42:08.8: 12.96 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:46:50.05 +37:10:02.6: 12.72 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:58:41.92 +40:42:08.8: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter KEPT candidate at 05:58:41.92 +40:42:08.8: ref_mag=12.98 +/- 0.02 new_mean_mag=11.8695 delta=1.11 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:46:50.05 +37:10:02.6: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 05:46:50.05 +37:10:02.6: ref_mag=12.80 +/- 0.01 new_mean_mag=11.8106 delta=0.99 (need > 0.90)
Adding exclusion_list_local.txt__out144454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out146725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74370.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 245227_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245227_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:34:07.69 +39:56:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245234_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245234_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:17:19.75 +39:28:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245238_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245238_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:17:58.02 +35:10:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245242_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245242_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:12:33.07 +36:57:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245246_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245246_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:19:49.23 +40:57:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245247_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245247_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:03:19.47 +36:32:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245249_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245249_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:03:00.57 +42:25:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245251_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245251_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:26:50.85 +38:58:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245252_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245252_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
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Considering the candidate 245253_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245253_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
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Considering the candidate 245254_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245254_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:04:36.87 +39:49:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245257_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245257_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:36:28.37 +34:07:21.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245363_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245363_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:19:15.64 +40:07:51.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245373_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245373_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:24:43.08 +37:25:06.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245381_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245381_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:50:57.96 +37:20:52.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245394_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245394_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:56:57.84 +33:05:59.1 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245424_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245424_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:27:41.47 +34:26:44.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245442_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245442_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:13:19.98 +38:30:50.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245454_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245454_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:19:00.80 +40:05:29.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245458_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245458_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:18:18.10 +33:47:33.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245459_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245459_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:00:16.18 +39:38:29.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245478_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245478_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:24:47.38 +37:21:51.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245483_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245483_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:18:54.64 +41:06:55.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245502_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245502_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:52:30.86 +36:43:05.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245512_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245512_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:56:56.87 +33:06:50.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245526_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245526_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:06:26.99 +41:12:20.6 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245529_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245529_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:10:27.46 +37:19:03.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245602_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245602_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 06:05:07.12 +37:56:46.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245608_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245608_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:52:57.80 +42:34:49.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245624_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245624_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:06:25.49 +34:49:29.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245627_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245627_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:06:28.51 +41:12:10.1 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245634_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245634_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:26:40.71 +34:23:15.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245679_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245679_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:13:44.48 +41:14:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245684_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245684_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245699_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245699_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245709_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245709_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:00:11.09 +39:24:18.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245715_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245715_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:24:35.29 +41:49:35.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245717_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245717_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:30:54.28 +39:49:17.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245723_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245723_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:19:01.52 +41:06:58.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245743_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245743_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:00:09.37 +39:38:54.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245755_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245755_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:18:29.76 +42:47:06.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245782_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245782_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245817_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245817_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245820_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245820_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:18:28.21 +37:36:36.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245831_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245831_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245841_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245841_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:06:33.93 +35:29:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245871_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 245871_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:58:54.57 +41:03:06.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49874_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 49874_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:26:53.85 +35:34:47.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44233_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 44233_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:20:55.58 +35:05:22.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42031_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 42031_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:02:26.23 +34:39:44.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50292_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 50292_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:25:29.53 +35:35:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114669_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 114669_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:20:15.00 +39:06:53.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39993_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 39993_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:36:12.77 +35:03:05.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133126_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 133126_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:24:55.81 +40:04:02.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146725_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
Preparing report for the candidate 146725_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93733_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 93733_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:56:05.88 +38:13:15.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 217102_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 217102_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:55:45.61 +41:06:24.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43591_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 43591_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:37:31.14 +35:17:00.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32333_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 32333_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:59:52.79 +33:59:11.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30548_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 30548_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:28:49.14 +34:25:09.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39924_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 39924_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:17:30.53 +34:49:22.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32190_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 32190_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:41:01.11 +34:37:15.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95220_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 95220_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:07:56.92 +37:48:57.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72927_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 72927_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:26:54.58 +36:54:11.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49989_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 49989_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:59:47.54 +35:03:03.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144454_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
Preparing report for the candidate 144454_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198845_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 198845_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:09:44.65 +40:44:24.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44411_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 44411_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 06:02:44.01 +35:19:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74370_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
Preparing report for the candidate 74370_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
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Considering the candidate 197929_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 197929_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 06:01:46.90 +41:06:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24314_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 24314_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:28:37.40 +34:02:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46899_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 46899_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:18:19.02 +35:14:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53361_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 53361_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:06:30.60 +35:23:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49281_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 49281_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:38:22.06 +35:37:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41258_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 41258_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:18:56.99 +34:57:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134108_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 134108_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 04:48:29.02 +39:16:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139440_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 139440_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:57:27.56 +40:27:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11737_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 11737_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:39:59.39 +33:26:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73667_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 73667_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:03:20.18 +36:34:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29050_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 29050_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:38:03.90 +34:25:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55043_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 55043_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:20:58.46 +35:48:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27184_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 27184_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 05:27:07.45 +34:08:59.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 123640_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 123640_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
**** FOUND 06:01:07.15 +39:40:14.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 96748_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417
The candidate 96748_fd_Aur-03-Q1b1x1_2026-07-28_04-25-43_20.00sec_-0.00C_LIGHTs_0417 did not pass the final checks
