This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT
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 03.3749 2461255.8749 12.79 05:33:34.42 +37:43:25.1
171.21957 2.54496 galactic Aur Second-epoch detections are separated by 2.2" and 8.5 pix
The object was found in VSX 1" NSVS J0533345+374322
Type: SR
# Max. Min./Amp. JD0 Period
13.231 r Y 0.884 r 2458469.47210 153.034937800000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:33:34.42 +37:43:25.1: 14.01 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:33:34.42 +37:43:25.1: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0533345+374322,2461255.8749,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0533345+374322 20260803.3749 12.79CV 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 03.3749 2461255.8749 12.91 05:12:40.10 +38:22:35.3
168.35363 -0.47998 galactic Aur Second-epoch detections are separated by 1.7" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.61 Danae -1 0 1 13.5 0 0
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:12:40.10 +38:22:35.3: 15.01 +/- 0.12 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:12:40.10 +38:22:35.3: 15.17 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.07 +/- 0.10
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,2461255.8749,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.3749 12.91CV 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 03.3749 2461255.8749 13.09 05:18:57.04 +34:57:09.0
171.87244 -1.44500 galactic Aur Second-epoch detections are separated by 1.2" and 8.0 pix
The object was found in VSX 1" OO Aur
Type: LB:
# Max. Min./Amp. JD0 Period
13.900 V 14.600 V C
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:18:57.04 +34:57:09.0: 14.17 +/- 0.09 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:18:57.04 +34:57:09.0: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.06
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
OO Aur,2461255.8749,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
OO Aur 20260803.3749 13.09CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461255.87515538 03.08.2026 09:00:03.425 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 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): 16551
Objects passed selection criteria: 16454
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 13270
Average stars matched: 11642.2 (87.7336 %)
Memory usage VmPeak: 246668 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 Mon Aug 3 04:19:36 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461255.87515538 03.08.2026 09:00:03.425 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 105
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 27 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): 129453
Objects passed selection criteria: 129110
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 110007
Average stars matched: 94938 (86.3018 %)
Memory usage VmPeak: 628492 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 Mon Aug 3 04:20:41 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.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: 2461255.87461405
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
Saving wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits to local_wcs_cache/
'wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits'
wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits exists and is non-empty
Saving wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits to local_wcs_cache/
'wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits'
wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits exists and is non-empty
Saving wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits to local_wcs_cache/
'wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits' -> 'local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits'
wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits exists and is non-empty
Saving wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits to local_wcs_cache/
'wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits' -> 'local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (1st reference image)
verification OK: wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:16.998 +37:59:58.58 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits (1st new image)
verification OK: wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
Image size: 941.0'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 05:27:14.580 +37:59:06.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:27:16.998 +37:59:58.58
Second-epoch image center 05:27:14.580 +37:59:06.16
Angular distance between the image centers 0.0166 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits (2nd new image)
verification OK: wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
Image size: 940.9'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 05:27:11.973 +37:58:29.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:27:16.998 +37:59:58.58
Second-epoch image center 05:27:11.973 +37:58:29.10
Angular distance between the image centers 0.0298 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:27:14.580 +37:59:06.16
Second-epoch second image center 05:27:11.973 +37:58:29.10
Angular distance between the image centers 0.01339 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.ZDPi8vsSxl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits &> /tmp/tmp.IyZVZHt0Tl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits &> /tmp/tmp.0oKkZ5BTsW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits &> /tmp/tmp.x0j3KguMfn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Found non-empty wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
The reference image (wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat) found
'wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat' -> 'wcsmag.cat'
Read 27843 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8756 to 92.1259 deg, Dec +31.9880 to +43.3913 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 70.8756 to 92.1259 deg, Dec 31.9880 to 43.3913 deg
Loaded 16034 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): 11109 out of 12457 total matches.
Matched with Tycho-2 12457 out of 27843 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.927300
a=0.000000 b=1.000000 c=22.927300
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 27843 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8756 to 92.1259 deg, Dec +31.9880 to +43.3913 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 70.8756 to 92.1259 deg, Dec 31.9880 to 43.3913 deg
Loaded 16034 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): 11109 out of 12457 total matches.
Matched with Tycho-2 12457 out of 27843 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Forced-photometry filter: calibrated wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (aperture=6.2)
Read 27116 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3491 to 92.6948 deg, Dec +32.1392 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 71.3491 to 92.6948 deg, Dec 32.1392 to 43.3190 deg
Loaded 16026 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): 11083 out of 12589 total matches.
Matched with Tycho-2 12589 out of 27116 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Forced-photometry filter: calibrated wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -> calib.txt_param_ref_wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
2.1 pix Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
2.3 pix fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
2.3 pix fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
Limiting magnitude estimates:
15.2 mag. Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
15.2 mag. Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
13.3 mag. fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
13.3 mag. fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 10.6 (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.ZDPi8vsSxl (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2982, bad_region=5998, passed=27843
Got 27843 stars (including 19362 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
util/solve_plate_with_UCAC5 got 27843 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4828 matched stars entering correct_measured_positions(), 4828 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4828 matched stars entering correct_measured_positions(), 23117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4827 matched stars entering correct_measured_positions(), 23117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4827 matched stars entering correct_measured_positions(), 23117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4827 stars left (next iteration limit 5310)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits N_match=4827 sigma_overall_arcsec=0.361 sigma_q1_arcsec=0.465 sigma_q2_arcsec=0.352 sigma_q3_arcsec=0.352 sigma_q4_arcsec=0.285 n_q1=1175 n_q2=1024 n_q3=1727 n_q4=901 worst_quadrant_to_overall_ratio=1.288
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.IyZVZHt0Tl (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3147, bad_region=5347, passed=27116
Got 27116 stars (including 19176 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
util/solve_plate_with_UCAC5 got 27116 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 4824 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4822 matched stars entering correct_measured_positions(), 23141 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 23141 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 23141 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4821 stars left (next iteration limit 5304)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits N_match=4821 sigma_overall_arcsec=0.533 sigma_q1_arcsec=0.654 sigma_q2_arcsec=0.497 sigma_q3_arcsec=0.485 sigma_q4_arcsec=0.487 n_q1=1354 n_q2=1041 n_q3=1564 n_q4=862 worst_quadrant_to_overall_ratio=1.228
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -region wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.0oKkZ5BTsW (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_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.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_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=371, bad_region=818, passed=5681
Got 5681 stars (including 4526 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat
util/solve_plate_with_UCAC5 got 5681 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 4441 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4363 matched stars entering correct_measured_positions(), 4368 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4363 matched stars entering correct_measured_positions(), 5032 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
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 43.3)
Done reading UCAC5 zone files...
Matched 4439 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4367 matched stars entering correct_measured_positions(), 5032 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 4367 matched stars entering correct_measured_positions(), 5032 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 4367 stars left (next iteration limit 4799)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4367 robust_rms=5.577 arcsec worst_quadrant_rms=7.553 arcsec
SIP_REFIT: SIP order 3 trial: matched=4367 robust_rms=0.658 arcsec worst_quadrant_rms=0.700 arcsec
SIP_REFIT: SIP order 5 trial: matched=4367 robust_rms=0.575 arcsec worst_quadrant_rms=0.640 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4367 robust_rms_before=1.748 arcsec robust_rms_before_corrected=0.593 arcsec robust_rms_after=0.575 arcsec worst_quadrant_rms_before=0.634 worst_quadrant_rms_after=0.640
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.634 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits N_match=4367 sigma_overall_arcsec=0.605 sigma_q1_arcsec=0.566 sigma_q2_arcsec=0.650 sigma_q3_arcsec=0.602 sigma_q4_arcsec=0.638 n_q1=1116 n_q2=761 n_q3=1746 n_q4=744 worst_quadrant_to_overall_ratio=1.075
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits -region wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.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.x0j3KguMfn (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_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.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_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=393, bad_region=835, passed=5692
Got 5692 stars (including 4501 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat
util/solve_plate_with_UCAC5 got 5692 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 4416 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4341 matched stars entering correct_measured_positions(), 4345 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4341 matched stars entering correct_measured_positions(), 5036 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
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 43.3)
Done reading UCAC5 zone files...
Matched 4414 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4344 matched stars entering correct_measured_positions(), 5036 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 4344 matched stars entering correct_measured_positions(), 5036 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 4344 stars left (next iteration limit 4775)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4344 robust_rms=5.631 arcsec worst_quadrant_rms=7.419 arcsec
SIP_REFIT: SIP order 3 trial: matched=4344 robust_rms=0.625 arcsec worst_quadrant_rms=0.663 arcsec
SIP_REFIT: SIP order 5 trial: matched=4344 robust_rms=0.550 arcsec worst_quadrant_rms=0.595 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4344 robust_rms_before=1.711 arcsec robust_rms_before_corrected=0.593 arcsec robust_rms_after=0.550 arcsec worst_quadrant_rms_before=0.629 worst_quadrant_rms_after=0.595
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.629 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits N_match=4344 sigma_overall_arcsec=0.603 sigma_q1_arcsec=0.578 sigma_q2_arcsec=0.616 sigma_q3_arcsec=0.634 sigma_q4_arcsec=0.623 n_q1=1084 n_q2=771 n_q3=1736 n_q4=753 worst_quadrant_to_overall_ratio=1.052
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits -region wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits sigma_overall=0.361 worst_q_ratio=1.288
ref2=Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits sigma_overall=0.533 worst_q_ratio=1.228
new1=fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits sigma_overall=0.605 worst_q_ratio=1.075
new2=fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits sigma_overall=0.603 worst_q_ratio=1.052
reference average sigma_overall=0.447 worst_q_ratio=1.258
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049_astrometric_residuals.png (4827 matched stars from wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054_astrometric_residuals.png (4821 matched stars from wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400_astrometric_residuals.png (4367 matched stars from wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.56 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401_astrometric_residuals.png (4344 matched stars from wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.56 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits'
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits'
Preparing the HTML report for the field Aur-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36485_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 36485_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:26:54.57 +36:54:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36487_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 36487_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:07:57.19 +37:48:57.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14476_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 14476_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:41:55.74 +38:55:59.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06908_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 06908_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:18:19.02 +35:14:59.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Aur-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Creating symlink local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits exists and is non-empty
wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits exists and is non-empty
wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (1st reference image)
verification OK: wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:16.998 +37:59:58.58 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits (1st new image)
verification OK: wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
Image size: 941.0'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 05:27:14.580 +37:59:06.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:27:16.998 +37:59:58.58
Second-epoch image center 05:27:14.580 +37:59:06.16
Angular distance between the image centers 0.0166 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits (2nd new image)
verification OK: wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
Image size: 940.9'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 05:27:11.973 +37:58:29.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:27:16.998 +37:59:58.58
Second-epoch image center 05:27:11.973 +37:58:29.10
Angular distance between the image centers 0.0298 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:27:14.580 +37:59:06.16
Second-epoch second image center 05:27:11.973 +37:58:29.10
Angular distance between the image centers 0.01339 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.BFLnfnGUpP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits &> /tmp/tmp.oconoxRWbg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits &> /tmp/tmp.x3iVNTQIc9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits &> /tmp/tmp.BIN8VdUcZA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Found non-empty wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
The reference image (wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat) found
'wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat' -> 'wcsmag.cat'
Read 202315 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8143 to 92.1485 deg, Dec +31.9880 to +43.3918 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 70.8143 to 92.1485 deg, Dec 31.9880 to 43.3918 deg
Loaded 16061 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): 8339 out of 12799 total matches.
Matched with Tycho-2 12799 out of 202315 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.774400
a=0.000000 b=1.000000 c=22.774400
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 202315 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8143 to 92.1485 deg, Dec +31.9880 to +43.3918 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 70.8143 to 92.1485 deg, Dec 31.9880 to 43.3918 deg
Loaded 16061 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): 8339 out of 12799 total matches.
Matched with Tycho-2 12799 out of 202315 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Forced-photometry filter: calibrated wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (aperture=4.6)
Read 212259 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3331 to 92.7203 deg, Dec +32.1392 to +43.3198 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 71.3331 to 92.7203 deg, Dec 32.1392 to 43.3198 deg
Loaded 16048 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): 8212 out of 12990 total matches.
Matched with Tycho-2 12990 out of 212259 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Forced-photometry filter: calibrated wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -> calib.txt_param_ref_wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 78 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
1.9 pix Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
2.1 pix fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
2.1 pix fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
Limiting magnitude estimates:
15.4 mag. Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
15.5 mag. Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
13.6 mag. fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
13.6 mag. fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 13.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.BFLnfnGUpP (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=30655, bad_region=36141, passed=202270
Got 202270 stars (including 139401 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
util/solve_plate_with_UCAC5 got 202270 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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 4834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 174446 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 174446 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 174447 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4834 stars left (next iteration limit 5317)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits N_match=4834 sigma_overall_arcsec=0.367 sigma_q1_arcsec=0.467 sigma_q2_arcsec=0.342 sigma_q3_arcsec=0.357 sigma_q4_arcsec=0.304 n_q1=1202 n_q2=1020 n_q3=1731 n_q4=881 worst_quadrant_to_overall_ratio=1.272
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.oconoxRWbg (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=32150, bad_region=35314, passed=212204
Got 212204 stars (including 148997 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
util/solve_plate_with_UCAC5 got 212204 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 4831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 185492 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4828 matched stars entering correct_measured_positions(), 185492 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 4828 matched stars entering correct_measured_positions(), 185492 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4828 stars left (next iteration limit 5313)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits N_match=4828 sigma_overall_arcsec=0.505 sigma_q1_arcsec=0.575 sigma_q2_arcsec=0.500 sigma_q3_arcsec=0.450 sigma_q4_arcsec=0.427 n_q1=1328 n_q2=1022 n_q3=1611 n_q4=867 worst_quadrant_to_overall_ratio=1.138
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -region wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.x3iVNTQIc9 (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_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.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_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2479, bad_region=5642, passed=54912
Got 54912 stars (including 46914 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat
util/solve_plate_with_UCAC5 got 54912 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 4898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 4822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 50841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
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 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 50841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 50841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 4823 stars left (next iteration limit 5300)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits N_match=4823 sigma_overall_arcsec=0.591 sigma_q1_arcsec=0.565 sigma_q2_arcsec=0.626 sigma_q3_arcsec=0.587 sigma_q4_arcsec=0.584 n_q1=1260 n_q2=786 n_q3=1910 n_q4=867 worst_quadrant_to_overall_ratio=1.059
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits -region wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.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.BIN8VdUcZA (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_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.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_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=2544, bad_region=5731, passed=55563
Got 55563 stars (including 47440 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat
util/solve_plate_with_UCAC5 got 55563 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 4816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 51436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
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 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 51436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 51436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 4816 stars left (next iteration limit 5294)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits N_match=4816 sigma_overall_arcsec=0.587 sigma_q1_arcsec=0.558 sigma_q2_arcsec=0.603 sigma_q3_arcsec=0.607 sigma_q4_arcsec=0.593 n_q1=1262 n_q2=799 n_q3=1877 n_q4=878 worst_quadrant_to_overall_ratio=1.034
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits -region wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.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_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/wcs_fd_Aur-03-Q2b1x1_2026-08-03_03-59-16_20.00sec_-0.00C_LIGHT_0400.fits
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.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_2026-08-03_CI_Aur-03-Q2b1x1_041703_TTUQ2b1x1_2870742_kaPyVtNT/wcs_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401.fits
Preparing the HTML report for the field Aur-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:03:18.34 +39:12:39.5: 12.79 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:24:29.40 +39:09:24.6: 12.91 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:45:58.92 +39:58:38.7: 12.55 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:02:12.76 +38:50:05.1: 12.66 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:36:20.84 +34:06:49.3: 12.25 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:34:29.03 +37:32:53.6: 12.92 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:50:25.68 +41:26:00.6: 12.55 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:34:00.32 +41:59:16.7: 12.27 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:04:22.65 +37:42:03.9: 12.53 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:02:12.76 +38:50:05.1: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:03:18.34 +39:12:39.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:45:58.92 +39:58:38.7: 12.61 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:36:20.84 +34:06:49.3: 12.30 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:34:29.03 +37:32:53.6: 12.82 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:24:29.40 +39:09:24.6: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.02
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry reference-image weighted average: 12.27 +/- 0.03
Forced photometry filter REJECTED candidate at 05:03:18.34 +39:12:39.5: ref_mag=12.79 +/- 0.02 new_mean_mag=12.8194 delta=-0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:02:12.76 +38:50:05.1: ref_mag=12.66 +/- 0.02 new_mean_mag=12.7968 delta=-0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:45:58.92 +39:58:38.7: ref_mag=12.58 +/- 0.01 new_mean_mag=12.8032 delta=-0.22 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:36:20.84 +34:06:49.3: ref_mag=12.27 +/- 0.03 new_mean_mag=12.7484 delta=-0.48 (need > 0.90)
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter REJECTED candidate at 05:34:29.03 +37:32:53.6: ref_mag=12.86 +/- 0.01 new_mean_mag=12.7727 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:24:29.40 +39:09:24.6: ref_mag=12.84 +/- 0.01 new_mean_mag=13.0808 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:50:25.68 +41:26:00.6: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.55 +/- 0.02
Forced photometry filter REJECTED candidate at 04:50:25.68 +41:26:00.6: ref_mag=12.55 +/- 0.02 new_mean_mag=12.7935 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:34:00.32 +41:59:16.7: 12.37 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:04:22.65 +37:42:03.9: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter REJECTED candidate at 05:34:00.32 +41:59:16.7: ref_mag=12.31 +/- 0.01 new_mean_mag=12.3916 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Forced photometry filter REJECTED candidate at 05:04:22.65 +37:42:03.9: ref_mag=12.53 +/- 0.01 new_mean_mag=12.6415 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:08:52.95 +38:02:24.0: 12.44 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:01:28.77 +40:30:31.8: 12.65 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:08:52.95 +38:02:24.0: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter REJECTED candidate at 05:08:52.95 +38:02:24.0: ref_mag=12.45 +/- 0.01 new_mean_mag=12.5311 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:58:31.43 +40:46:21.9: 9.73 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:01:28.77 +40:30:31.8: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.65 +/- 0.03
Forced photometry filter REJECTED candidate at 05:01:28.77 +40:30:31.8: ref_mag=12.65 +/- 0.03 new_mean_mag=12.4937 delta=0.16 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:01:10.73 +41:14:48.5: 12.77 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:58:31.43 +40:46:21.9: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 9.73 +/- 0.00
Forced photometry filter REJECTED candidate at 04:58:31.43 +40:46:21.9: ref_mag=9.73 +/- 0.00 new_mean_mag=10.1131 delta=-0.38 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:24:49.98 +37:22:47.9: 12.66 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:58:54.66 +41:03:07.1: 13.03 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:01:10.73 +41:14:48.5: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 12.77 +/- 0.03
Forced photometry filter REJECTED candidate at 05:01:10.73 +41:14:48.5: ref_mag=12.77 +/- 0.03 new_mean_mag=12.7245 delta=0.04 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:06.04 +39:18:43.1: 13.14 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:24:49.98 +37:22:47.9: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter REJECTED candidate at 05:24:49.98 +37:22:47.9: ref_mag=12.61 +/- 0.01 new_mean_mag=12.5106 delta=0.10 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:58:54.66 +41:03:07.1: 99.00 +/- 99.00 bad_region
Forced photometry reference-image weighted average: 13.03 +/- 0.03
Forced photometry filter REJECTED candidate at 04:58:54.66 +41:03:07.1: ref_mag=13.03 +/- 0.03 new_mean_mag=12.9185 delta=0.11 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:06.04 +39:18:43.1: 13.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.04
Forced photometry filter REJECTED candidate at 05:20:06.04 +39:18:43.1: ref_mag=13.16 +/- 0.04 new_mean_mag=12.8462 delta=0.31 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:33:34.42 +37:43:25.1: 14.01 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:12:40.10 +38:22:35.3: 15.01 +/- 0.12 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:33:34.42 +37:43:25.1: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.03
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:12:40.10 +38:22:35.3: 15.17 +/- 0.15 detection
Forced photometry filter KEPT candidate at 05:33:34.42 +37:43:25.1: ref_mag=13.83 +/- 0.03 new_mean_mag=12.7648 delta=1.07 (need > 0.90)
Forced photometry reference-image weighted average: 15.07 +/- 0.10
Forced photometry filter KEPT candidate at 05:12:40.10 +38:22:35.3: ref_mag=15.07 +/- 0.10 new_mean_mag=12.9123 delta=2.16 (need > 0.90)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:18:57.04 +34:57:09.0: 14.17 +/- 0.09 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:18:57.04 +34:57:09.0: 13.99 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.06
Forced photometry filter KEPT candidate at 05:18:57.04 +34:57:09.0: ref_mag=14.06 +/- 0.06 new_mean_mag=13.0526 delta=1.01 (need > 0.90)
Adding exclusion_list_local.txt__out102587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85851.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 271929_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271929_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 271945_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271945_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 271946_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271946_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 271958_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271958_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 271968_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271968_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 271969_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271969_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 271971_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271971_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:17:58.08 +35:10:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271976_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271976_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:10:49.54 +41:58:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271977_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271977_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:15:57.41 +39:12:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271978_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271978_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:28:38.07 +39:14:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271981_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271981_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 271982_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271982_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 271983_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271983_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:06:05.50 +41:39:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271984_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271984_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 271985_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271985_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:14:49.65 +39:31:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271986_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271986_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 271989_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271989_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
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Considering the candidate 271992_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271992_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:36:28.05 +34:07:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 271993_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271993_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:26:50.92 +38:58:32.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271994_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271994_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:19:49.29 +40:57:01.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 271995_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 271995_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:01:46.77 +37:33:13.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272000_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272000_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:04:36.92 +39:49:46.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272005_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272005_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272039_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272039_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:19:15.64 +40:07:51.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272090_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272090_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:24:43.06 +37:25:06.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272094_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272094_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:13:19.91 +38:30:51.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272137_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272137_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:10:27.44 +37:19:04.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272139_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272139_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:00:16.31 +39:38:29.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272143_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272143_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:27:41.45 +34:26:44.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272150_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272150_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:18:18.12 +33:47:34.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272161_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272161_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:49:06.79 +39:13:06.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272169_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272169_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:24:47.39 +37:21:50.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272186_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272186_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:06:25.47 +34:49:30.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272190_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272190_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:19:01.61 +41:06:58.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272203_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272203_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:17:19.70 +39:28:43.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272226_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272226_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272256_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272256_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:45:51.22 +37:37:55.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272269_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272269_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272270_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272270_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:19:59.42 +39:20:10.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272271_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272271_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:30:54.23 +39:49:16.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272280_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272280_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:14:24.39 +39:22:48.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272282_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272282_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:00:11.09 +39:24:17.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272284_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272284_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272286_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272286_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:18:28.41 +37:36:36.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272292_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272292_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:26:40.70 +34:23:15.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272303_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272303_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:32:38.92 +39:32:29.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272308_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272308_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:18:37.33 +37:44:43.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272321_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272321_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:13:46.56 +41:12:08.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272327_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272327_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272338_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272338_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:29:49.47 +35:22:28.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272339_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272339_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:13:15.98 +40:10:22.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272347_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272347_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:00:09.22 +39:38:55.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272358_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272358_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:09:36.36 +38:39:30.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272365_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272365_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:14:45.18 +39:31:19.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272366_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272366_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:06:24.79 +41:11:55.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272373_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272373_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:06:33.97 +35:29:43.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272417_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272417_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:18:40.09 +39:21:05.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272419_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272419_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:28:31.77 +35:56:44.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272435_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272435_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:22:17.22 +37:03:24.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272440_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272440_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:30:43.09 +39:51:59.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272444_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272444_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:15:38.65 +38:20:30.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272447_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272447_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:10:18.42 +40:22:52.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 272453_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 272453_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:20:43.59 +37:24:54.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85851_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
Preparing report for the candidate 85851_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96748_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 96748_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:20:45.12 +38:10:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102587_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
Preparing report for the candidate 102587_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114669_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 114669_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:20:15.16 +39:06:51.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133126_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 133126_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:24:55.89 +40:04:01.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32190_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 32190_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:41:01.19 +34:37:14.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95220_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 95220_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:07:57.16 +37:48:57.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72927_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 72927_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:26:54.60 +36:54:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86440_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 86440_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:30:32.91 +37:44:46.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49989_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 49989_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 04:59:47.72 +35:03:04.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198845_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 198845_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:09:44.71 +40:44:23.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46899_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 46899_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:18:19.04 +35:15:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111430_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 111430_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks
**** FOUND 05:41:55.74 +38:55:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41258_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
Preparing report for the candidate 41258_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
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Considering the candidate 73667_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401
The candidate 73667_fd_Aur-03-Q2b1x1_2026-08-03_04-00-03_20.00sec_-0.00C_LIGHT_0401 did not pass the final checks