This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj
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 28.3949 2461249.8949 12.30 06:12:04.03 +42:31:22.4
170.70871 11.30699 galactic Aur Second-epoch detections are separated by 1.5" and 7.5 pix
The object was found in VSX 1" ASASSN-V J061204.00+423121.9
Type: L
# Max. Min./Amp. JD0 Period
13.120 V 13.750 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 06:12:04.03 +42:31:22.4: 13.20 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 06:12:04.03 +42:31:22.4: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 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 J061204.00+423121.9,2461249.8949,12.30,0.05,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 J061204.00+423121.9 20260728.3949 12.30CV 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 28.3949 2461249.8949 12.71 05:50:06.30 +46:03:39.9
165.65816 9.49975 galactic Aur Second-epoch detections are separated by 3.0" and 7.8 pix
The object was found in VSX 1" ASASSN-V J055006.23+460340.0
Type: SRS
# Max. Min./Amp. JD0 Period
14.900 g Y 0.300 g 2458386.88900 23.867000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:50:06.30 +46:03:39.9: 13.74 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:50:06.30 +46:03:39.9: 13.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J055006.23+460340.0,2461249.8949,12.71,0.05,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 J055006.23+460340.0 20260728.3949 12.71CV 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 28.3949 2461249.8949 12.15 06:06:06.70 +41:11:06.1
171.40470 9.70973 galactic Aur Second-epoch detections are separated by 1.9" and 7.1 pix
The object was found in VSX 1" ASASSN-V J060606.67+411105.2
Type: L
# Max. Min./Amp. JD0 Period
13.650 V 13.890 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 06:06:06.70 +41:11:06.1: 13.27 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 06:06:06.70 +41:11:06.1: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 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 J060606.67+411105.2,2461249.8949,12.15,0.05,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 J060606.67+411105.2 20260728.3949 12.15CV 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 28.3949 2461249.8949 12.06 06:11:29.40 +42:19:24.8
170.84163 11.12238 galactic Aur Second-epoch detections are separated by 0.5" and 7.2 pix
The object was found in VSX 1" V0375 Aur
Type: SR
# Max. Min./Amp. JD0 Period
14.600 pg 15.600 pg 2443736.00000 510.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 06:11:29.40 +42:19:24.8: 13.04 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 06:11:29.40 +42:19:24.8: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 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
V0375 Aur,2461249.8949,12.06,0.05,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
V0375 Aur 20260728.3949 12.06CV 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 28.3949 2461249.8949 11.31 05:33:25.96 +41:34:34.8
167.95935 4.60834 galactic Aur Second-epoch detections are separated by 0.8" and 7.9 pix
The object was found in VSX 2" ASASSN-V J053325.78+413434.6
Type: L:
# Max. Min./Amp. JD0 Period
12.850 V 13.390 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:33:25.96 +41:34:34.8: 12.21 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:33:25.96 +41:34:34.8: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 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
ASASSN-V J053325.78+413434.6,2461249.8949,11.31,0.05,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 J053325.78+413434.6 20260728.3949 11.31CV 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 28.3949 2461249.8949 11.06 06:13:22.47 +47:44:24.7
166.00676 13.79973 galactic Aur Second-epoch detections are separated by 0.3" and 7.1 pix
The object was found in VSX 1" SS Aur
Type: UGSS
# Max. Min./Amp. JD0 Period
10.300 V 16.800 V 0.182800000000 M3-5Ve
The object was not found in astcheck.
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 06:13:22.47 +47:44:24.7: 12.14 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 06:13:22.47 +47:44:24.7: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 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
SS Aur,2461249.8949,11.06,0.05,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
SS Aur 20260728.3949 11.06CV 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: 2461058.73146802 18.01.2026 05:33:08.837 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
First image: 2461058.73146802 18.01.2026 05:33:08.837 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
Last image: 2461249.89523578 28.07.2026 09:28:58.371 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
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: 10 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): 24022
Objects passed selection criteria: 23856
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 14799.8
Average stars matched: 14362 (97.0422 %)
Memory usage VmPeak: 248616 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 05:59:33 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: 2461058.73146802 18.01.2026 05:33:08.837 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
First image: 2461058.73146802 18.01.2026 05:33:08.837 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
Last image: 2461249.89523578 28.07.2026 09:28:58.371 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 67
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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: 32 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): 162136
Objects passed selection criteria: 161649
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: 106035
Average stars matched: 102060 (96.2517 %)
Memory usage VmPeak: 626476 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 06:11:23 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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.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: 2461249.89463643
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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits exists and is non-empty
Saving wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits to local_wcs_cache/
'wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits' -> 'local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits'
wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits exists and is non-empty
Saving wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits to local_wcs_cache/
'wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits' -> 'local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits'
wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits'
wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits (1st reference image)
verification OK: wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:01.120 +45:59:31.34 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-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:06.285 +46:00:10.05 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:00:01.120 +45:59:31.34
Second-epoch image center 06:00:06.285 +46:00:10.05
Angular distance between the image centers 0.0184 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
Image size: 944.9'x626.9' 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: 06:00:09.281 +45:59:38.96 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:00:01.120 +45:59:31.34
Second-epoch image center 06:00:09.281 +45:59:38.96
Angular distance between the image centers 0.0237 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:00:06.285 +46:00:10.05
Second-epoch second image center 06:00:09.281 +45:59:38.96
Angular distance between the image centers 0.01224 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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits &> /tmp/tmp.CFmKksC3BY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits &> /tmp/tmp.Y1N71ZpqhF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits &> /tmp/tmp.8lzqa8PDEK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits &> /tmp/tmp.7tmvKDB8vC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits and wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits and wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits and wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat
The reference image (wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits) and catalog (wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat) found
'wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat' -> 'wcsmag.cat'
Read 25793 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.9795 to 102.6262 deg, Dec +39.9539 to +51.3305 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 77.9795 to 102.6262 deg, Dec 39.9539 to 51.3305 deg
Loaded 11869 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): 7971 out of 8928 total matches.
Matched with Tycho-2 8928 out of 25793 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.931400
a=0.000000 b=1.000000 c=22.931400
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 25793 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.9795 to 102.6262 deg, Dec +39.9539 to +51.3305 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 77.9795 to 102.6262 deg, Dec 39.9539 to 51.3305 deg
Loaded 11869 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): 7971 out of 8928 total matches.
Matched with Tycho-2 8928 out of 25793 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits:
Forced-photometry filter: calibrated wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits -> calib.txt_param_ref_wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits (aperture=6.2)
Read 25835 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.9795 to 102.6261 deg, Dec +39.9544 to +51.3404 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 77.9795 to 102.6261 deg, Dec 39.9544 to 51.3404 deg
Loaded 11878 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): 7967 out of 8927 total matches.
Matched with Tycho-2 8927 out of 25835 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits:
Forced-photometry filter: calibrated wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits -> calib.txt_param_ref_wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
2.2 pix Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
2.6 pix fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
2.6 pix fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
2.2 pix wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
2.2 pix wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
Limiting magnitude estimates:
15.4 mag. Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
15.4 mag. Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
12.9 mag. fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
12.9 mag. fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 10.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.CFmKksC3BY (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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.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=2509, bad_region=0, passed=25793
Got 25793 stars (including 23250 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat
util/solve_plate_with_UCAC5 got 25793 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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 4857 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 4819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 25793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 4856 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 25793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 25793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4818 stars left (next iteration limit 5299)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits N_match=4818 sigma_overall_arcsec=0.383 sigma_q1_arcsec=0.475 sigma_q2_arcsec=0.375 sigma_q3_arcsec=0.330 sigma_q4_arcsec=0.342 n_q1=1013 n_q2=1164 n_q3=1194 n_q4=1447 worst_quadrant_to_overall_ratio=1.242
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits -region wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.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.Y1N71ZpqhF (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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.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-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.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-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits.wcscat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits.wcscat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.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=2498, bad_region=0, passed=25835
Got 25835 stars (including 23302 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits.wcscat
util/solve_plate_with_UCAC5 got 25835 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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 4856 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 4818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 25835 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 4856 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 25835 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 25835 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4816 stars left (next iteration limit 5297)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits N_match=4816 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.426 sigma_q2_arcsec=0.385 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.336 n_q1=1014 n_q2=1162 n_q3=1187 n_q4=1453 worst_quadrant_to_overall_ratio=1.115
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits -region wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.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.8lzqa8PDEK (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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.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=285, bad_region=0, passed=4027
Got 4027 stars (including 3735 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat
util/solve_plate_with_UCAC5 got 4027 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 3617 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3578 matched stars entering correct_measured_positions(), 3579 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3578 matched stars entering correct_measured_positions(), 4027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 3617 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3577 matched stars entering correct_measured_positions(), 4027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 3577 matched stars entering correct_measured_positions(), 4027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 3577 stars left (next iteration limit 3935)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3577 robust_rms=9.474 arcsec worst_quadrant_rms=13.653 arcsec
SIP_REFIT: SIP order 3 trial: matched=3577 robust_rms=0.612 arcsec worst_quadrant_rms=1.145 arcsec
SIP_REFIT: SIP order 5 trial: matched=3577 robust_rms=0.429 arcsec worst_quadrant_rms=0.577 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3577 robust_rms_before=1.606 arcsec robust_rms_before_corrected=0.478 arcsec robust_rms_after=0.429 arcsec worst_quadrant_rms_before=0.646 worst_quadrant_rms_after=0.577
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
Image size: 945.3'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:06.426 +46:00:08.20 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 4027 stars ###
'wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/correct_sextractor_wcs_catalog_usingxy2sky2309685.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.606 -> 0.429 arcsec)
WCS_QUALITY_DIAG: file=fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits N_match=3577 sigma_overall_arcsec=0.455 sigma_q1_arcsec=0.455 sigma_q2_arcsec=0.633 sigma_q3_arcsec=0.361 sigma_q4_arcsec=0.439 n_q1=1009 n_q2=744 n_q3=990 n_q4=834 worst_quadrant_to_overall_ratio=1.392
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits -region wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.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.7tmvKDB8vC (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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits.wcscat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits.wcscat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.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=266, bad_region=0, passed=3966
Got 3966 stars (including 3690 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits.wcscat
util/solve_plate_with_UCAC5 got 3966 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.9'
Seting catalog search parameters based on the expected field of view 944.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013124 (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 0.010499 (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 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 3575 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3532 matched stars entering correct_measured_positions(), 3532 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3532 matched stars entering correct_measured_positions(), 3966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 3575 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3532 matched stars entering correct_measured_positions(), 3966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 3532 matched stars entering correct_measured_positions(), 3966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 3532 stars left (next iteration limit 3885)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3532 robust_rms=9.756 arcsec worst_quadrant_rms=13.170 arcsec
SIP_REFIT: SIP order 3 trial: matched=3532 robust_rms=0.727 arcsec worst_quadrant_rms=1.154 arcsec
SIP_REFIT: SIP order 5 trial: matched=3532 robust_rms=0.478 arcsec worst_quadrant_rms=0.679 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3532 robust_rms_before=1.589 arcsec robust_rms_before_corrected=0.473 arcsec robust_rms_after=0.478 arcsec worst_quadrant_rms_before=0.582 worst_quadrant_rms_after=0.679
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.582 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits N_match=3532 sigma_overall_arcsec=0.476 sigma_q1_arcsec=0.461 sigma_q2_arcsec=0.590 sigma_q3_arcsec=0.382 sigma_q4_arcsec=0.457 n_q1=975 n_q2=740 n_q3=973 n_q4=844 worst_quadrant_to_overall_ratio=1.241
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits -region wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits sigma_overall=0.383 worst_q_ratio=1.242
ref2=Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits sigma_overall=0.382 worst_q_ratio=1.115
new1=fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits sigma_overall=0.455 worst_q_ratio=1.392
new2=fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits sigma_overall=0.476 worst_q_ratio=1.241
reference average sigma_overall=0.3825 worst_q_ratio=1.1785
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220_astrometric_residuals.png (4818 matched stars from wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221_astrometric_residuals.png (4816 matched stars from wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420_astrometric_residuals.png (3577 matched stars from wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421_astrometric_residuals.png (3532 matched stars from wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits'
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31705_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 31705_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:09:52.05 +46:34:28.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31707_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 31707_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:57:23.93 +48:22:41.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10156_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 10156_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:34:13.53 +45:57:59.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02446_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 02446_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:27:04.54 +50:07:26.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18275_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 18275_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:12:08.18 +43:09:51.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09794_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 09794_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:27:25.47 +46:15:59.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00922_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 00922_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:26:01.98 +50:29:29.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
Creating symlink local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits exists and is non-empty
wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits (1st reference image)
verification OK: wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:01.120 +45:59:31.34 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-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:06.285 +46:00:10.05 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:00:01.120 +45:59:31.34
Second-epoch image center 06:00:06.285 +46:00:10.05
Angular distance between the image centers 0.0184 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
Image size: 944.9'x626.9' 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: 06:00:09.281 +45:59:38.96 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:00:01.120 +45:59:31.34
Second-epoch image center 06:00:09.281 +45:59:38.96
Angular distance between the image centers 0.0237 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:00:06.285 +46:00:10.05
Second-epoch second image center 06:00:09.281 +45:59:38.96
Angular distance between the image centers 0.01224 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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits &> /tmp/tmp.ROfkqxPfPF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits &> /tmp/tmp.zjLXEucNWK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits &> /tmp/tmp.bWKPyoJGuv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits &> /tmp/tmp.ciYYIk1jGk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits and wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits and wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits and wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat
The reference image (wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits) and catalog (wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat) found
'wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat' -> 'wcsmag.cat'
Read 179065 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.9271 to 102.6825 deg, Dec +39.9455 to +51.3354 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 77.9271 to 102.6825 deg, Dec 39.9455 to 51.3354 deg
Loaded 11941 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): 6304 out of 8978 total matches.
Matched with Tycho-2 8978 out of 179065 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.800650
a=0.000000 b=1.000000 c=22.800650
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.53
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 179065 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.9271 to 102.6825 deg, Dec +39.9455 to +51.3354 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 77.9271 to 102.6825 deg, Dec 39.9455 to 51.3354 deg
Loaded 11941 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): 6304 out of 8978 total matches.
Matched with Tycho-2 8978 out of 179065 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits:
Forced-photometry filter: calibrated wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits -> calib.txt_param_ref_wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits (aperture=4.7)
Read 177912 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.9443 to 102.6826 deg, Dec +39.9474 to +51.3466 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 77.9443 to 102.6826 deg, Dec 39.9474 to 51.3466 deg
Loaded 11934 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): 6278 out of 8977 total matches.
Matched with Tycho-2 8977 out of 177912 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits:
Forced-photometry filter: calibrated wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits -> calib.txt_param_ref_wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 59 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
2.1 pix Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
2.5 pix fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
2.5 pix fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
2.0 pix wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
2.1 pix wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
Limiting magnitude estimates:
15.5 mag. Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
15.5 mag. Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
13.2 mag. fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
13.2 mag. fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.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.ROfkqxPfPF (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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.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-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.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=59, blended=22508, bad_region=2, passed=179006
Got 179006 stars (including 156229 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat
util/solve_plate_with_UCAC5 got 179006 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 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4843 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 4809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 179006 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4843 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 179006 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 179006 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4809 stars left (next iteration limit 5289)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits N_match=4809 sigma_overall_arcsec=0.369 sigma_q1_arcsec=0.435 sigma_q2_arcsec=0.364 sigma_q3_arcsec=0.315 sigma_q4_arcsec=0.313 n_q1=1014 n_q2=1196 n_q3=1191 n_q4=1408 worst_quadrant_to_overall_ratio=1.179
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits -region wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.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.zjLXEucNWK (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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.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-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.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-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits.wcscat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits.wcscat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.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=70, blended=22509, bad_region=0, passed=177842
Got 177842 stars (including 155045 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits.wcscat
util/solve_plate_with_UCAC5 got 177842 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 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4845 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(), 4815 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 177842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4845 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 177842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 177842 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4812 stars left (next iteration limit 5294)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits N_match=4812 sigma_overall_arcsec=0.362 sigma_q1_arcsec=0.410 sigma_q2_arcsec=0.351 sigma_q3_arcsec=0.322 sigma_q4_arcsec=0.325 n_q1=1002 n_q2=1198 n_q3=1193 n_q4=1419 worst_quadrant_to_overall_ratio=1.134
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits -region wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.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.bWKPyoJGuv (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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1283, bad_region=2, passed=35132
Got 35132 stars (including 33792 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat
util/solve_plate_with_UCAC5 got 35132 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 4847 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 4799 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 35132 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 4847 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4802 matched stars entering correct_measured_positions(), 35132 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4802 matched stars entering correct_measured_positions(), 35132 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4802 stars left (next iteration limit 5277)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits N_match=4802 sigma_overall_arcsec=0.445 sigma_q1_arcsec=0.469 sigma_q2_arcsec=0.565 sigma_q3_arcsec=0.358 sigma_q4_arcsec=0.424 n_q1=1322 n_q2=934 n_q3=1436 n_q4=1110 worst_quadrant_to_overall_ratio=1.271
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits -region wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.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.ciYYIk1jGk (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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits.wcscat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits.wcscat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.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=1257, bad_region=1, passed=34680
Got 34680 stars (including 33362 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits.wcscat
util/solve_plate_with_UCAC5 got 34680 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.9'
Seting catalog search parameters based on the expected field of view 944.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013124 (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 0.010499 (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 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 4857 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4805 matched stars entering correct_measured_positions(), 4806 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4805 matched stars entering correct_measured_positions(), 34680 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 4857 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 34680 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 34680 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4809 stars left (next iteration limit 5285)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits N_match=4809 sigma_overall_arcsec=0.455 sigma_q1_arcsec=0.469 sigma_q2_arcsec=0.541 sigma_q3_arcsec=0.383 sigma_q4_arcsec=0.450 n_q1=1318 n_q2=943 n_q3=1437 n_q4=1111 worst_quadrant_to_overall_ratio=1.189
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Aur-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits -region wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.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-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-06_20.00sec_-0.00C_LIGHTs_0420.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.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-02-Q1b1x1_050825_TTUQ1b1x1_209625_KbjVJ4Vj/wcs_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421.fits
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:28:11.27 +45:21:58.6: 11.33 +/- 0.00 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 06:30:48.16 +40:18:59.4: 11.75 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:24:09.83 +47:19:02.3: 12.66 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 06:20:51.25 +40:57:13.9: 12.30 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:26:36.90 +44:48:48.8: 11.66 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:43:27.54 +42:19:24.3: 11.00 +/- 0.00 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:16:23.06 +45:56:32.8: 11.76 +/- 0.08 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:24:09.83 +47:19:02.3: 12.69 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:28:11.27 +45:21:58.6: 11.35 +/- 0.00 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 06:30:48.16 +40:18:59.4: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry reference-image weighted average: 11.34 +/- 0.00
Forced photometry filter REJECTED candidate at 05:28:11.27 +45:21:58.6: ref_mag=11.34 +/- 0.00 new_mean_mag=11.3872 delta=-0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:24:09.83 +47:19:02.3: ref_mag=12.68 +/- 0.01 new_mean_mag=12.5396 delta=0.14 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 06:20:51.25 +40:57:13.9: 12.31 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:26:36.90 +44:48:48.8: 11.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Forced photometry filter REJECTED candidate at 06:30:48.16 +40:18:59.4: ref_mag=11.77 +/- 0.01 new_mean_mag=11.9551 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:43:27.54 +42:19:24.3: 10.99 +/- 0.00 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry reference-image weighted average: 11.69 +/- 0.00
Forced photometry filter REJECTED candidate at 06:20:51.25 +40:57:13.9: ref_mag=12.31 +/- 0.01 new_mean_mag=11.9290 delta=0.38 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:26:36.90 +44:48:48.8: ref_mag=11.69 +/- 0.00 new_mean_mag=11.9667 delta=-0.27 (need > 0.90)
Forced photometry reference-image weighted average: 11.00 +/- 0.00
Forced photometry filter REJECTED candidate at 05:43:27.54 +42:19:24.3: ref_mag=11.00 +/- 0.00 new_mean_mag=11.2121 delta=-0.22 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:16:23.06 +45:56:32.8: 11.83 +/- 0.09 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.06
Forced photometry filter REJECTED candidate at 05:16:23.06 +45:56:32.8: ref_mag=11.79 +/- 0.06 new_mean_mag=11.8982 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:51:47.71 +48:44:50.8: 12.27 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:25:37.50 +45:40:54.6: 12.13 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:46:26.66 +47:55:00.6: 12.48 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:35:43.79 +47:10:30.9: 12.50 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 06:13:16.49 +48:28:25.2: 12.90 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:51:47.71 +48:44:50.8: 12.31 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:25:37.50 +45:40:54.6: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry filter REJECTED candidate at 05:51:47.71 +48:44:50.8: ref_mag=12.29 +/- 0.01 new_mean_mag=12.3029 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter REJECTED candidate at 05:25:37.50 +45:40:54.6: ref_mag=12.13 +/- 0.01 new_mean_mag=12.1773 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:40:02.72 +50:02:05.3: 12.84 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:58:04.35 +45:06:13.4: 12.49 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:35:43.79 +47:10:30.9: 12.48 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:46:26.66 +47:55:00.6: 12.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter REJECTED candidate at 05:35:43.79 +47:10:30.9: ref_mag=12.49 +/- 0.01 new_mean_mag=12.3097 delta=0.18 (need > 0.90)
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter REJECTED candidate at 05:46:26.66 +47:55:00.6: ref_mag=12.49 +/- 0.01 new_mean_mag=12.4318 delta=0.06 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 06:13:16.49 +48:28:25.2: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.01
Forced photometry filter REJECTED candidate at 06:13:16.49 +48:28:25.2: ref_mag=12.91 +/- 0.01 new_mean_mag=12.6078 delta=0.30 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:40:02.72 +50:02:05.3: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Forced photometry filter REJECTED candidate at 05:40:02.72 +50:02:05.3: ref_mag=12.86 +/- 0.02 new_mean_mag=12.8563 delta=0.00 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:58:04.35 +45:06:13.4: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter REJECTED candidate at 05:58:04.35 +45:06:13.4: ref_mag=12.49 +/- 0.01 new_mean_mag=12.3629 delta=0.12 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 06:12:04.03 +42:31:22.4: 13.20 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:50:06.30 +46:03:39.9: 13.74 +/- 0.04 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 06:12:04.03 +42:31:22.4: 13.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 06:12:04.03 +42:31:22.4: ref_mag=13.19 +/- 0.02 new_mean_mag=12.2789 delta=0.91 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 06:38:10.56 +40:12:16.4: 11.79 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 06:06:06.70 +41:11:06.1: 13.27 +/- 0.03 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:50:06.30 +46:03:39.9: 13.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.03
Forced photometry filter KEPT candidate at 05:50:06.30 +46:03:39.9: ref_mag=13.69 +/- 0.03 new_mean_mag=12.7031 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 06:11:29.40 +42:19:24.8: 13.04 +/- 0.02 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 06:38:10.56 +40:12:16.4: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Forced photometry filter REJECTED candidate at 06:38:10.56 +40:12:16.4: ref_mag=11.79 +/- 0.01 new_mean_mag=11.8791 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 06:06:06.70 +41:11:06.1: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 06:06:06.70 +41:11:06.1: ref_mag=13.29 +/- 0.02 new_mean_mag=12.1466 delta=1.15 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 06:34:29.69 +40:38:57.2: 12.00 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 06:11:29.40 +42:19:24.8: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.01
Forced photometry filter KEPT candidate at 06:11:29.40 +42:19:24.8: ref_mag=13.04 +/- 0.01 new_mean_mag=12.0583 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 06:34:29.69 +40:38:57.2: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry filter REJECTED candidate at 06:34:29.69 +40:38:57.2: ref_mag=12.00 +/- 0.01 new_mean_mag=11.9071 delta=0.09 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 05:33:25.96 +41:34:34.8: 12.21 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-33-08_20.00sec_-15.00C_LIGHT_0220.fits at 06:13:22.47 +47:44:24.7: 12.14 +/- 0.01 detection
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 05:33:25.96 +41:34:34.8: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter KEPT candidate at 05:33:25.96 +41:34:34.8: ref_mag=12.23 +/- 0.01 new_mean_mag=11.2884 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aur-02-Q1b1x1_2026-01-17_23-34-12_20.00sec_-15.00C_LIGHT_0221.fits at 06:13:22.47 +47:44:24.7: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter KEPT candidate at 06:13:22.47 +47:44:24.7: ref_mag=12.13 +/- 0.01 new_mean_mag=11.0622 delta=1.07 (need > 0.90)
Adding exclusion_list_local.txt__out132178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82259.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 204189_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204189_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 204192_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204192_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:37:23.83 +44:31:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204196_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204196_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:15:15.57 +49:13:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204197_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204197_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:33:05.04 +47:49:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204198_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204198_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 204203_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204203_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 204207_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204207_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 204208_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204208_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:28:39.65 +41:12:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204210_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204210_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 204211_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204211_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 204247_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204247_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:13:42.11 +45:31:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204270_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204270_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:59:43.44 +44:59:09.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 204317_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204317_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:47:13.08 +42:30:25.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204323_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204323_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 204325_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204325_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:27:49.79 +48:14:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204350_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204350_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:11:34.51 +48:44:34.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204380_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204380_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:17:53.29 +49:34:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204387_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204387_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 204391_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204391_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:47:46.85 +48:48:04.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204406_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204406_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 204417_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204417_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:59:57.65 +45:53:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204424_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204424_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 204437_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204437_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:39:19.67 +42:40:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204450_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204450_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 204467_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204467_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:00:05.64 +51:06:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204469_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204469_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:00:57.30 +47:55:59.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204494_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204494_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 204498_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204498_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:18:23.63 +48:55:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204509_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204509_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 204510_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204510_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 204635_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204635_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:53:12.09 +45:24:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 204645_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 204645_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:57:46.15 +45:53:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135863_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
Preparing report for the candidate 135863_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
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Considering the candidate 78454_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 78454_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:48:25.48 +46:18:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65788_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 65788_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:14:59.06 +46:47:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82259_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
Preparing report for the candidate 82259_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
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Considering the candidate 143029_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 143029_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:16:01.06 +42:50:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154770_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 154770_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 124041_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 124041_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:38:54.84 +43:45:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71477_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 71477_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:09:52.02 +46:34:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159446_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
Preparing report for the candidate 159446_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
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Considering the candidate 57551_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 57551_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:55:40.02 +47:30:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49732_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 49732_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:43:00.66 +47:58:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 132178_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
Preparing report for the candidate 132178_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
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Considering the candidate 48498_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 48498_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:54:00.57 +48:02:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159933_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 159933_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
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Considering the candidate 06146_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 06146_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:26:01.92 +50:29:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78557_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 78557_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:26:59.15 +45:47:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100804_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 100804_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:41:12.63 +44:10:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72707_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 72707_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:49:32.31 +46:35:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16109_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 16109_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:27:04.56 +50:07:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147852_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 147852_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:12:08.21 +43:09:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164773_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
Preparing report for the candidate 164773_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
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Considering the candidate 50597_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
Preparing report for the candidate 50597_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
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Considering the candidate 68390_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 68390_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:40:36.06 +46:53:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43009_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 43009_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 05:57:23.94 +48:22:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73430_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 73430_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:34:13.51 +45:57:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71979_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 71979_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
**** FOUND 06:27:25.43 +46:15:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162585_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421
The candidate 162585_fd_Aur-02-Q1b1x1_2026-07-28_04-28-58_20.00sec_0.00C_LIGHTs_0421 did not pass the final checks
