This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu
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 08 02.4233 2461254.9233 11.68 06:14:13.59 +33:26:32.9
179.09744 7.54138 galactic Aur Second-epoch detections are separated by 1.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.89 Julia 0 -0 0 11.6 0 0
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:14:13.59 +33:26:32.9: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:14:13.59 +33:26:32.9: 16.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461254.9233,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260802.4233 11.68CV 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 08 02.4233 2461254.9233 12.09 06:47:14.21 +35:21:03.8
180.32066 14.50827 galactic Gem Second-epoch detections are separated by 4.3" and 7.5 pix
The object was found in VSX 1" NSVS J0647143+352105
Type: L:
# Max. Min./Amp. JD0 Period
11.043 R1 Y 0.574 R1 149.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:47:14.21 +35:21:03.8: 13.14 +/- 0.02 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:47:14.21 +35:21:03.8: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 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
NSVS J0647143+352105,2461254.9233,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0647143+352105 20260802.4233 12.09CV 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 08 02.4233 2461254.9233 11.66 06:43:16.48 +39:04:27.2
176.45580 15.23710 galactic Aur Second-epoch detections are separated by 1.1" and 6.7 pix
The object was found in VSX 2" ASASSN-V J064316.38+390428.2
Type: L
# Max. Min./Amp. JD0 Period
12.480 V 13.040 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:43:16.48 +39:04:27.2: 12.72 +/- 0.01 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:43:16.48 +39:04:27.2: 12.74 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.73 +/- 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 J064316.38+390428.2,2461254.9233,11.66,0.05,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 J064316.38+390428.2 20260802.4233 11.66CV 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 08 02.4233 2461254.9233 10.98 06:58:24.35 +37:05:24.8
179.53516 17.25182 galactic Aur Second-epoch detections are separated by 1.1" and 6.9 pix
The object was found in VSX 3" NSVS J0658245+370523
Type: L:
# Max. Min./Amp. JD0 Period
10.217 R1 Y 0.323 R1 60.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:58:24.35 +37:05:24.8: 12.09 +/- 0.01 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:58:24.35 +37:05:24.8: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 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
NSVS J0658245+370523,2461254.9233,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0658245+370523 20260802.4233 10.98CV 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 08 02.4233 2461254.9233 10.81 07:00:28.77 +40:20:54.5
176.48047 18.78221 galactic Aur Second-epoch detections are separated by 1.9" and 6.8 pix
The object was found in VSX 2" ASASSN-V J070028.89+402055.6
Type: L
# Max. Min./Amp. JD0 Period
11.770 V 12.420 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 07:00:28.77 +40:20:54.5: 11.72 +/- 0.01 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 07:00:28.77 +40:20:54.5: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.74 +/- 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 J070028.89+402055.6,2461254.9233,10.81,0.05,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 J070028.89+402055.6 20260802.4233 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.73457257 18.01.2026 05:37:37.070 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
First image: 2461058.73457257 18.01.2026 05:37:37.070 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Last image: 2461254.92367741 02.08.2026 10:09:55.728 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 22939
Objects passed selection criteria: 22747
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: 14045.5
Average stars matched: 13666.8 (97.3034 %)
Memory usage VmPeak: 248288 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 2 05:13:53 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.73457257 18.01.2026 05:37:37.070 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
First image: 2461058.73457257 18.01.2026 05:37:37.070 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Last image: 2461254.92367741 02.08.2026 10:09:55.728 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 65
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 28 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 151482
Objects passed selection criteria: 151021
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: 96729.5
Average stars matched: 92540.2 (95.6691 %)
Memory usage VmPeak: 616388 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 2 05:15:09 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
SExtractor catalog cache: saved Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.cat to cache
SExtractor catalog cache: saved Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.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: 2461254.92292594
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits exists and is non-empty
Saving wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits to local_wcs_cache/
'wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits' -> 'local_wcs_cache/wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits'
wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits exists and is non-empty
Saving wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits to local_wcs_cache/
'wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits' -> 'local_wcs_cache/wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits'
wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits exists and is non-empty
Saving wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits to local_wcs_cache/
'wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits' -> 'local_wcs_cache/wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits'
wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits exists and is non-empty
Saving wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits to local_wcs_cache/
'wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits' -> 'local_wcs_cache/wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits (1st reference image)
verification OK: wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Image size: 941.7'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:32:42.831 +37:59:58.61 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits (1st new image)
verification OK: wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
Image size: 945.1'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:32:45.267 +38:01:19.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:32:42.831 +37:59:58.61
Second-epoch image center 06:32:45.267 +38:01:19.23
Angular distance between the image centers 0.0238 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits (2nd new image)
verification OK: wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:32:43.222 +38:00:47.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:32:42.831 +37:59:58.61
Second-epoch image center 06:32:43.222 +38:00:47.92
Angular distance between the image centers 0.0138 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:32:45.267 +38:01:19.23
Second-epoch second image center 06:32:43.222 +38:00:47.92
Angular distance between the image centers 0.01099 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits &> /tmp/tmp.69wwXlgtPB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits &> /tmp/tmp.SGY2HvrEBk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits &> /tmp/tmp.rWaf6c9cGE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits &> /tmp/tmp.mPI5fHAKLz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits and wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits and wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
Found non-empty wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits and wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
The reference image (wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits) and catalog (wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat) found
'wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat' -> 'wcsmag.cat'
Read 24697 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.6955 to 109.0154 deg, Dec +32.1587 to +43.3191 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 87.6955 to 109.0154 deg, Dec 32.1587 to 43.3191 deg
Loaded 14448 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): 10172 out of 11254 total matches.
Matched with Tycho-2 11254 out of 24697 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.927300
a=0.000000 b=1.000000 c=22.927300
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.37
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 24697 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.6955 to 109.0154 deg, Dec +32.1587 to +43.3191 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 87.6955 to 109.0154 deg, Dec 32.1587 to 43.3191 deg
Loaded 14448 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): 10172 out of 11254 total matches.
Matched with Tycho-2 11254 out of 24697 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Forced-photometry filter: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits -> calib.txt_param_ref_wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits (aperture=6.2)
Read 24494 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.6934 to 109.0157 deg, Dec +32.1588 to +43.3190 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 87.6934 to 109.0157 deg, Dec 32.1588 to 43.3190 deg
Loaded 14450 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): 10148 out of 11235 total matches.
Matched with Tycho-2 11235 out of 24494 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
Forced-photometry filter: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits -> calib.txt_param_ref_wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
2.2 pix Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
2.9 pix fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
2.9 pix fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
Limiting magnitude estimates:
15.4 mag. Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
15.4 mag. Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
12.8 mag. fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
12.8 mag. fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
All-image limiting magnitude estimate: 12.8 (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.69wwXlgtPB (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_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits' -> 'wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
WCS-calibrated image found: wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Checking if the catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
WCS catalog name: wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2296, bad_region=0, passed=24697
Got 24697 stars (including 22379 good ones) from the SExtractor catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
util/solve_plate_with_UCAC5 got 24697 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4815 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 4773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 24697 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4815 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4771 matched stars entering correct_measured_positions(), 24697 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4771 matched stars entering correct_measured_positions(), 24697 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4771 stars left (next iteration limit 5249)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits N_match=4771 sigma_overall_arcsec=0.324 sigma_q1_arcsec=0.384 sigma_q2_arcsec=0.339 sigma_q3_arcsec=0.294 sigma_q4_arcsec=0.301 n_q1=1081 n_q2=1269 n_q3=1120 n_q4=1301 worst_quadrant_to_overall_ratio=1.186
The image catalog is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits -region wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.SGY2HvrEBk (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_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits' -> 'wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
Checking if the catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
WCS catalog name: wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2308, bad_region=0, passed=24494
Got 24494 stars (including 22154 good ones) from the SExtractor catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat
util/solve_plate_with_UCAC5 got 24494 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4813 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4766 matched stars entering correct_measured_positions(), 4766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4766 matched stars entering correct_measured_positions(), 24494 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4813 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4764 matched stars entering correct_measured_positions(), 24494 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4764 matched stars entering correct_measured_positions(), 24494 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4764 stars left (next iteration limit 5242)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits N_match=4764 sigma_overall_arcsec=0.362 sigma_q1_arcsec=0.445 sigma_q2_arcsec=0.373 sigma_q3_arcsec=0.312 sigma_q4_arcsec=0.333 n_q1=1060 n_q2=1285 n_q3=1120 n_q4=1299 worst_quadrant_to_overall_ratio=1.231
The image catalog is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits -region wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.rWaf6c9cGE (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_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.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_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
Checking if the catalog wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
WCS catalog name: wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.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=171, bad_region=0, passed=3651
Got 3651 stars (including 3476 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits.wcscat
util/solve_plate_with_UCAC5 got 3651 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.1'
Seting catalog search parameters based on the expected field of view 945.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013126 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010501 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 669 (Dec 32.3 to 43.4)
Done reading UCAC5 zone files...
Matched 3338 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3299 matched stars entering correct_measured_positions(), 3300 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3299 matched stars entering correct_measured_positions(), 3650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 611 to 669 (Dec 32.3 to 43.4)
Done reading UCAC5 zone files...
Matched 3340 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3299 matched stars entering correct_measured_positions(), 3650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 3298 matched stars entering correct_measured_positions(), 3650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 3298 stars left (next iteration limit 3628)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3298 robust_rms=6.727 arcsec worst_quadrant_rms=21.077 arcsec
SIP_REFIT: SIP order 3 trial: matched=3298 robust_rms=0.592 arcsec worst_quadrant_rms=1.329 arcsec
SIP_REFIT: SIP order 5 trial: matched=3298 robust_rms=0.495 arcsec worst_quadrant_rms=0.691 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3298 robust_rms_before=1.540 arcsec robust_rms_before_corrected=0.510 arcsec robust_rms_after=0.495 arcsec worst_quadrant_rms_before=0.732 worst_quadrant_rms_after=0.691
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.732 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits N_match=3298 sigma_overall_arcsec=0.482 sigma_q1_arcsec=0.530 sigma_q2_arcsec=0.650 sigma_q3_arcsec=0.364 sigma_q4_arcsec=0.476 n_q1=1049 n_q2=475 n_q3=1146 n_q4=628 worst_quadrant_to_overall_ratio=1.347
The image catalog is written to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits -region wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.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.mPI5fHAKLz (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_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.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_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
Checking if the catalog wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
WCS catalog name: wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.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=170, bad_region=0, passed=3687
Got 3687 stars (including 3512 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat
util/solve_plate_with_UCAC5 got 3687 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 611 to 668 (Dec 32.3 to 43.4)
Done reading UCAC5 zone files...
Matched 3379 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3348 matched stars entering correct_measured_positions(), 3349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3348 matched stars entering correct_measured_positions(), 3686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 611 to 668 (Dec 32.3 to 43.4)
Done reading UCAC5 zone files...
Matched 3381 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3346 matched stars entering correct_measured_positions(), 3687 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 3346 matched stars entering correct_measured_positions(), 3687 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 3346 stars left (next iteration limit 3682)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3346 robust_rms=6.908 arcsec worst_quadrant_rms=18.437 arcsec
SIP_REFIT: SIP order 3 trial: matched=3346 robust_rms=0.618 arcsec worst_quadrant_rms=1.264 arcsec
SIP_REFIT: SIP order 5 trial: matched=3346 robust_rms=0.516 arcsec worst_quadrant_rms=0.790 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3346 robust_rms_before=1.566 arcsec robust_rms_before_corrected=0.524 arcsec robust_rms_after=0.516 arcsec worst_quadrant_rms_before=0.728 worst_quadrant_rms_after=0.790
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.728 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits N_match=3346 sigma_overall_arcsec=0.497 sigma_q1_arcsec=0.513 sigma_q2_arcsec=0.682 sigma_q3_arcsec=0.393 sigma_q4_arcsec=0.524 n_q1=1058 n_q2=487 n_q3=1154 n_q4=647 worst_quadrant_to_overall_ratio=1.372
The image catalog is written to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits -region wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits sigma_overall=0.324 worst_q_ratio=1.186
ref2=Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits sigma_overall=0.362 worst_q_ratio=1.231
new1=fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits sigma_overall=0.482 worst_q_ratio=1.347
new2=fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits sigma_overall=0.497 worst_q_ratio=1.372
reference average sigma_overall=0.343 worst_q_ratio=1.2085
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224_astrometric_residuals.png (4771 matched stars from wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225_astrometric_residuals.png (4764 matched stars from wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200_astrometric_residuals.png (3298 matched stars from wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201_astrometric_residuals.png (3346 matched stars from wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.45 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits'
Saving fully-calibrated image wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits'
Preparing the HTML report for the field Aur-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06765_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 06765_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:30:55.93 +40:17:00.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10445_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 10445_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:43:57.47 +38:29:20.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12672_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 12672_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:33:49.19 +37:35:42.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07955_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 07955_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:01:07.28 +39:40:14.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22918_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 22918_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:52:47.05 +33:57:40.4 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Aur-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
SExtractor catalog cache: saved Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.cat to cache
SExtractor catalog cache: saved Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Creating symlink local_wcs_cache/wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits exists and is non-empty
wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits exists and is non-empty
wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits exists and is non-empty
wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits exists and is non-empty
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# fov_of_wcs_calibrated_image.sh output for wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits (1st reference image)
verification OK: wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Image size: 941.7'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:32:42.831 +37:59:58.61 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits (1st new image)
verification OK: wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
Image size: 945.1'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:32:45.267 +38:01:19.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:32:42.831 +37:59:58.61
Second-epoch image center 06:32:45.267 +38:01:19.23
Angular distance between the image centers 0.0238 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits (2nd new image)
verification OK: wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:32:43.222 +38:00:47.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:32:42.831 +37:59:58.61
Second-epoch image center 06:32:43.222 +38:00:47.92
Angular distance between the image centers 0.0138 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:32:45.267 +38:01:19.23
Second-epoch second image center 06:32:43.222 +38:00:47.92
Angular distance between the image centers 0.01099 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits &> /tmp/tmp.jOF340koZq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits &> /tmp/tmp.H4xdYutsyB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits &> /tmp/tmp.gi1e2kHLPw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits &> /tmp/tmp.YIxppU5KOU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits and wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits and wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
Found non-empty wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits and wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
The reference image (wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits) and catalog (wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat) found
'wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat' -> 'wcsmag.cat'
Read 164929 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.6716 to 109.0154 deg, Dec +32.1587 to +43.3211 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 87.6716 to 109.0154 deg, Dec 32.1587 to 43.3211 deg
Loaded 14475 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): 8144 out of 11406 total matches.
Matched with Tycho-2 11406 out of 164929 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.799100
a=0.000000 b=1.000000 c=22.799100
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 164929 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.6716 to 109.0154 deg, Dec +32.1587 to +43.3211 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 87.6716 to 109.0154 deg, Dec 32.1587 to 43.3211 deg
Loaded 14475 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): 8144 out of 11406 total matches.
Matched with Tycho-2 11406 out of 164929 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Forced-photometry filter: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits -> calib.txt_param_ref_wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits (aperture=4.8)
Read 167662 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.6638 to 109.0157 deg, Dec +32.1588 to +43.3199 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 87.6638 to 109.0157 deg, Dec 32.1588 to 43.3199 deg
Loaded 14479 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): 8103 out of 11406 total matches.
Matched with Tycho-2 11406 out of 167662 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
Forced-photometry filter: calibrated wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits -> calib.txt_param_ref_wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 59 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
2.0 pix Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
2.8 pix fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
2.8 pix fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
Limiting magnitude estimates:
15.5 mag. Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
15.5 mag. Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
13.0 mag. fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
13.1 mag. fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 12.6 (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.jOF340koZq (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_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits' -> 'wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
WCS-calibrated image found: wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
Checking if the catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits
WCS catalog name: wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=53, blended=19895, bad_region=2, passed=164876
Got 164876 stars (including 144720 good ones) from the SExtractor catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat
util/solve_plate_with_UCAC5 got 164876 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4798 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4764 matched stars entering correct_measured_positions(), 4765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4764 matched stars entering correct_measured_positions(), 164876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4798 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4763 matched stars entering correct_measured_positions(), 164876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4763 matched stars entering correct_measured_positions(), 164876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4763 stars left (next iteration limit 5240)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits N_match=4763 sigma_overall_arcsec=0.317 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.335 sigma_q3_arcsec=0.285 sigma_q4_arcsec=0.294 n_q1=1113 n_q2=1252 n_q3=1148 n_q4=1250 worst_quadrant_to_overall_ratio=1.082
The image catalog is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits -region wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.H4xdYutsyB (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_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits' -> 'wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
Checking if the catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits
WCS catalog name: wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=49, blended=20373, bad_region=1, passed=167613
Got 167613 stars (including 146982 good ones) from the SExtractor catalog wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat
util/solve_plate_with_UCAC5 got 167613 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4800 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4770 matched stars entering correct_measured_positions(), 4770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4770 matched stars entering correct_measured_positions(), 167613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4800 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4769 matched stars entering correct_measured_positions(), 167613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4769 matched stars entering correct_measured_positions(), 167613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4769 stars left (next iteration limit 5247)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits N_match=4769 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.408 sigma_q2_arcsec=0.368 sigma_q3_arcsec=0.303 sigma_q4_arcsec=0.318 n_q1=1102 n_q2=1255 n_q3=1160 n_q4=1252 worst_quadrant_to_overall_ratio=1.165
The image catalog is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits -region wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.gi1e2kHLPw (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_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.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_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
Checking if the catalog wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
WCS catalog name: wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.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=2, blended=1060, bad_region=3, passed=28081
Got 28081 stars (including 26973 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits.wcscat
util/solve_plate_with_UCAC5 got 28081 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.1'
Seting catalog search parameters based on the expected field of view 945.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013126 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010501 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4805 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4748 matched stars entering correct_measured_positions(), 4752 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4748 matched stars entering correct_measured_positions(), 28080 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4807 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4745 matched stars entering correct_measured_positions(), 28080 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4745 matched stars entering correct_measured_positions(), 28080 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4745 stars left (next iteration limit 5222)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits N_match=4745 sigma_overall_arcsec=0.500 sigma_q1_arcsec=0.541 sigma_q2_arcsec=0.693 sigma_q3_arcsec=0.405 sigma_q4_arcsec=0.504 n_q1=1464 n_q2=660 n_q3=1701 n_q4=920 worst_quadrant_to_overall_ratio=1.387
The image catalog is written to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits -region wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.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.YIxppU5KOU (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_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.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_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
Checking if the catalog wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
WCS catalog name: wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.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=5, blended=1087, bad_region=3, passed=28876
Got 28876 stars (including 27736 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat
util/solve_plate_with_UCAC5 got 28876 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4809 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4758 matched stars entering correct_measured_positions(), 4763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4758 matched stars entering correct_measured_positions(), 28875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 669 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 4810 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4756 matched stars entering correct_measured_positions(), 28875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 4756 matched stars entering correct_measured_positions(), 28875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 4756 stars left (next iteration limit 5233)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits N_match=4756 sigma_overall_arcsec=0.494 sigma_q1_arcsec=0.525 sigma_q2_arcsec=0.649 sigma_q3_arcsec=0.404 sigma_q4_arcsec=0.516 n_q1=1457 n_q2=669 n_q3=1708 n_q4=922 worst_quadrant_to_overall_ratio=1.313
The image catalog is written to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits -region wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.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_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-08-50_20.00sec_-0.00C_LIGHTs_0200.fits
Saving fully-calibrated image wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.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_2026-08-02_CI_Aur-04-Q1b1x1_051114_TTUQ1b1x1_174589_rtzQCsGu/wcs_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201.fits
Preparing the HTML report for the field Aur-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:14:13.59 +33:26:32.9: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:24:37.25 +35:14:12.2: 11.84 +/- 0.01 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:14:13.59 +33:26:32.9: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:24:37.25 +35:14:12.2: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Forced photometry filter REJECTED candidate at 06:24:37.25 +35:14:12.2: ref_mag=11.83 +/- 0.01 new_mean_mag=11.8205 delta=0.01 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:47:14.21 +35:21:03.8: 13.14 +/- 0.02 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:43:16.48 +39:04:27.2: 12.72 +/- 0.01 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:47:14.21 +35:21:03.8: 13.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 06:47:14.21 +35:21:03.8: ref_mag=13.14 +/- 0.02 new_mean_mag=12.0920 delta=1.05 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 06:58:24.35 +37:05:24.8: 12.09 +/- 0.01 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:43:16.48 +39:04:27.2: 12.74 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 06:43:16.48 +39:04:27.2: ref_mag=12.73 +/- 0.01 new_mean_mag=11.6599 delta=1.07 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 06:58:24.35 +37:05:24.8: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry filter KEPT candidate at 06:58:24.35 +37:05:24.8: ref_mag=12.11 +/- 0.01 new_mean_mag=10.9884 delta=1.12 (need > 0.90)
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-37-37_20.00sec_-14.90C_LIGHT_0224.fits at 07:00:28.77 +40:20:54.5: 11.72 +/- 0.01 detection
Forced photometry on wcs_Aur-04-Q1b1x1_2026-01-17_23-38-14_20.00sec_-14.90C_LIGHT_0225.fits at 07:00:28.77 +40:20:54.5: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.74 +/- 0.01
Forced photometry filter KEPT candidate at 07:00:28.77 +40:20:54.5: ref_mag=11.74 +/- 0.01 new_mean_mag=10.8100 delta=0.93 (need > 0.90)
Adding exclusion_list_local.txt__out144172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out190735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89082.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 190546_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190546_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:13:16.73 +40:32:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190554_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190554_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:09:22.89 +41:45:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190557_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190557_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:32:09.68 +34:19:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190559_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190559_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:02:05.01 +42:27:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190662_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190662_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:09:41.43 +37:12:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190735_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
Preparing report for the candidate 190735_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
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Considering the candidate 190736_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190736_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:05:00.59 +42:57:34.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190740_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190740_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 05:59:31.65 +37:13:41.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 190772_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190772_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:09:09.90 +34:55:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190777_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190777_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:05:07.17 +37:56:46.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190815_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190815_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:06:07.56 +35:21:22.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190823_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190823_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
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Considering the candidate 190824_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190824_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:08:07.15 +37:57:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190861_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190861_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:06:09.54 +39:36:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190932_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190932_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:13:27.69 +37:08:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190959_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190959_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:01:11.68 +41:56:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190993_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 190993_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:30:07.30 +38:57:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191012_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 191012_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:08:19.97 +41:02:08.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 191085_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 191085_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:15:09.02 +39:55:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191166_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 191166_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:11:41.30 +42:07:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70567_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 70567_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:43:57.43 +38:29:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09087_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 09087_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:33:59.95 +42:35:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131653_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 131653_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:02:50.51 +34:41:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138329_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 138329_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:05:32.83 +35:07:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142823_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 142823_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:02:37.97 +35:22:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10740_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 10740_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
Rejecting candidate due to large distance (38.0") between the two second-epoch detections
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Considering the candidate 106238_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 106238_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:06:00.48 +36:20:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129129_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 129129_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:33:14.43 +34:30:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102748_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 102748_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:08:53.62 +36:35:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160071_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 160071_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:38:32.67 +33:21:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 144172_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
Preparing report for the candidate 144172_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
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Considering the candidate 31406_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 31406_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
Rejecting candidate due to large distance (38.4") between the two second-epoch detections
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Considering the candidate 142365_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 142365_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:02:44.45 +35:19:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31752_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 31752_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:15:48.55 +41:02:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163572_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 163572_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:33:11.51 +33:40:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111281_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 111281_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:28:02.05 +36:04:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60331_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
Preparing report for the candidate 60331_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
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Considering the candidate 117019_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 117019_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:41:52.90 +33:41:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110958_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 110958_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:15:09.60 +36:08:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129951_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 129951_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:18:22.94 +34:38:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89082_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
Preparing report for the candidate 89082_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
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Considering the candidate 109892_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 109892_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:34:13.51 +36:10:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97991_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 97991_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:02:30.76 +36:52:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38681_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 38681_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:07:44.05 +40:31:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36603_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
Preparing report for the candidate 36603_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
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Considering the candidate 43810_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 43810_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:30:55.93 +40:17:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87216_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 87216_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:33:49.20 +37:35:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51937_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 51937_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:01:07.26 +39:40:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156552_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 156552_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:17:14.48 +33:12:25.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 72371_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 72371_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:36:32.81 +38:26:40.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 58107_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 58107_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:38:39.35 +39:23:21.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 113862_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 113862_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:53:03.42 +35:47:16.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 86217_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 86217_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:57:18.40 +37:23:40.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 07770_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 07770_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:39:19.73 +42:29:14.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 16613_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 16613_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 06:50:45.72 +41:46:46.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 128647_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 128647_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:07:22.45 +34:00:32.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 135753_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 135753_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:06:11.44 +34:28:24.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 49483_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 49483_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
**** FOUND 07:11:39.21 +39:19:12.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 123113_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201
The candidate 123113_fd_Aur-04-Q1b1x1_2026-08-02_05-09-55_20.00sec_-0.00C_LIGHTs_0201 did not pass the final checks
