This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 23.4458 2461244.9458 11.80 05:53:00.98 +33:33:30.3
176.84317 3.72959 galactic Aur Second-epoch detections are separated by 1.6" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.89 Julia -1 0 1 11.5 0 0
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:53:00.98 +33:33:30.3: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:53:00.98 +33:33:30.3: 16.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461244.9458,11.80,0.05,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 20260723.4458 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 23.4458 2461244.9458 12.75 05:53:52.92 +26:15:26.5
183.23853 0.19392 galactic Tau Second-epoch detections are separated by 0.9" and 9.5 pix
The object was found in VSX 7" Gaia DR3 3430637945528992896
Type: ROT
# Max. Min./Amp. JD0 Period
15.940 G 15.990 G G
NOTE: the measured brightness disagrees with the variable-star record above, but is consistent with the asteroid identification below - so this is likely the asteroid rather than an outburst of the variable.
The object was found in astcheck.111 Ate -1 1 1 13.4 0 0
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:53:52.92 +26:15:26.5: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:53:52.92 +26:15:26.5: 15.83 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.83 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 23.4458* 05 53 52.92 +26 15 26.5 12.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3430637945528992896,2461244.9458,12.75,0.05,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
Gaia DR3 3430637945528992896 20260723.4458 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 23.4458 2461244.9458 12.21 05:46:15.94 +31:13:33.6
178.11707 1.31073 galactic Aur Second-epoch detections are separated by 1.3" and 9.4 pix
The object was found in VSX22" Gaia DR3 3445002480827933056
Type: E
# Max. Min./Amp. JD0 Period
19.210 G 19.870 G 50.170000000000
NOTE: the measured brightness disagrees with the variable-star record above, but is consistent with the asteroid identification below - so this is likely the asteroid rather than an outburst of the variable.
The object was found in astcheck.250 Bettina -3 1 3 13.3 0 0
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:46:15.94 +31:13:33.6: 13.31 +/- 0.03 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:46:15.94 +31:13:33.6: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3445002480827933056,2461244.9458,12.21,0.05,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
Gaia DR3 3445002480827933056 20260723.4458 12.21CV 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: 2461093.61992316 22.02.2026 02:52:31.361 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
First image: 2461093.61992316 22.02.2026 02:52:31.361 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Last image: 2461244.94612784 23.07.2026 10:42:15.445 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
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: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 21061
Objects passed selection criteria: 20905
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 13005.5
Average stars matched: 12252.8 (94.2121 %)
Memory usage VmPeak: 129356 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 22 16:05:55 CDT 2026
VaST build number 1.0rc89-166-g55a66cb7
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-22)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 23 09:09:24 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: 2461093.61992316 22.02.2026 02:52:31.361 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
First image: 2461093.61992316 22.02.2026 02:52:31.361 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Last image: 2461244.94612784 23.07.2026 10:42:15.445 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 75
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
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: 41 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 171155
Objects passed selection criteria: 170607
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 112190
Average stars matched: 104956 (93.5518 %)
Memory usage VmPeak: 1935776 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 22 16:05:55 CDT 2026
VaST build number 1.0rc89-166-g55a66cb7
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-22)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 23 09:15:31 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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
SExtractor catalog cache: saved Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.cat to cache
SExtractor catalog cache: saved Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.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: 2461244.94556060
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits exists and is non-empty
Saving wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits to local_wcs_cache/
'wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits' -> 'local_wcs_cache/wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits'
wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits exists and is non-empty
Saving wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits to local_wcs_cache/
'wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits' -> 'local_wcs_cache/wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits'
wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits exists and is non-empty
Saving wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits to local_wcs_cache/
'wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits' -> 'local_wcs_cache/wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits'
wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits exists and is non-empty
Saving wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits to local_wcs_cache/
'wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits' -> 'local_wcs_cache/wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits (1st reference image)
verification OK: wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:00.480 +29:59:52.07 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-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits (1st new image)
verification OK: wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
Image size: 940.7'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 06:00:24.969 +30:02:29.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:00:00.480 +29:59:52.07
Second-epoch image center 06:00:24.969 +30:02:29.56
Angular distance between the image centers 0.0986 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits (2nd new image)
verification OK: wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
Image size: 940.7'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 06:00:28.120 +30:01:50.98 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:00:00.480 +29:59:52.07
Second-epoch image center 06:00:28.120 +30:01:50.98
Angular distance between the image centers 0.1051 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:00:24.969 +30:02:29.56
Second-epoch second image center 06:00:28.120 +30:01:50.98
Angular distance between the image centers 0.01562 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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits &> /tmp/tmp.fIuyUEN779
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits &> /tmp/tmp.f8eqwx46xr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits &> /tmp/tmp.0pFgjhDozX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits &> /tmp/tmp.ZOM4k3ExVF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits and wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits and wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat
Found non-empty wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits and wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat
The reference image (wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits) and catalog (wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat) found
'wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat' -> 'wcsmag.cat'
Read 27193 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.5801 to 99.6659 deg, Dec +24.3425 to +35.3069 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 80.5801 to 99.6659 deg, Dec 24.3425 to 35.3069 deg
Loaded 17091 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): 11926 out of 13489 total matches.
Matched with Tycho-2 13489 out of 27193 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.939750
a=0.000000 b=1.000000 c=22.939750
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.24
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.24
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 27193 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.5801 to 99.6659 deg, Dec +24.3425 to +35.3069 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 80.5801 to 99.6659 deg, Dec 24.3425 to 35.3069 deg
Loaded 17091 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): 11926 out of 13489 total matches.
Matched with Tycho-2 13489 out of 27193 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits:
Forced-photometry filter: calibrated wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits -> calib.txt_param_ref_wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits (aperture=6.0)
Read 27141 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.5948 to 99.6661 deg, Dec +24.3432 to +35.3120 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 80.5948 to 99.6661 deg, Dec 24.3432 to 35.3120 deg
Loaded 17084 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): 12065 out of 13603 total matches.
Matched with Tycho-2 13603 out of 27141 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits:
Forced-photometry filter: calibrated wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits -> calib.txt_param_ref_wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
2.1 pix Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
2.3 pix fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
2.4 pix fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
2.1 pix wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
2.1 pix wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
Limiting magnitude estimates:
15.2 mag. Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
15.2 mag. Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
13.2 mag. fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
13.1 mag. fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
All-image limiting magnitude estimate: 13.1 (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.fIuyUEN779 (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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits' -> 'wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
WCS_IMAGE_NAME=wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
WCS-calibrated image found: wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Checking if the catalog wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat corresponding to the image wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits alredy exist and is non-empty...
Catalog wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat corresponding to the image wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
WCS catalog name: wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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=3136, bad_region=5792, passed=27193
Got 27193 stars (including 18877 good ones) from the SExtractor catalog wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat
util/solve_plate_with_UCAC5 got 27193 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 21813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 21813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 21812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits N_match=928 sigma_overall_arcsec=0.484 sigma_q1_arcsec=0.587 sigma_q2_arcsec=0.415 sigma_q3_arcsec=0.471 sigma_q4_arcsec=0.455 n_q1=231 n_q2=198 n_q3=280 n_q4=219 worst_quadrant_to_overall_ratio=1.214
The image catalog is written to wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits -region wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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.f8eqwx46xr (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-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits' -> 'wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
WCS-calibrated image found: wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
Checking if the catalog wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
WCS catalog name: wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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=3121, bad_region=5776, passed=27141
Got 27141 stars (including 18855 good ones) from the SExtractor catalog wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
util/solve_plate_with_UCAC5 got 27141 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 21919 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 21918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 21918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits N_match=934 sigma_overall_arcsec=0.471 sigma_q1_arcsec=0.565 sigma_q2_arcsec=0.442 sigma_q3_arcsec=0.471 sigma_q4_arcsec=0.418 n_q1=241 n_q2=198 n_q3=278 n_q4=217 worst_quadrant_to_overall_ratio=1.201
The image catalog is written to wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits -region wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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.0pFgjhDozX (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
WCS_IMAGE_NAME=wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
WCS-calibrated image found: wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
Checking if the catalog wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
WCS catalog name: wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.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=387, bad_region=880, passed=5712
Got 5712 stars (including 4484 good ones) from the SExtractor catalog wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits.wcscat
util/solve_plate_with_UCAC5 got 5712 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.7'
Seting catalog search parameters based on the expected field of view 940.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013065 (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 0.010452 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 4857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 4859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 4859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits N_match=929 sigma_overall_arcsec=0.551 sigma_q1_arcsec=0.566 sigma_q2_arcsec=0.518 sigma_q3_arcsec=0.610 sigma_q4_arcsec=0.515 n_q1=291 n_q2=151 n_q3=346 n_q4=141 worst_quadrant_to_overall_ratio=1.108
The image catalog is written to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits -region wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.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.ZOM4k3ExVF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
WCS_IMAGE_NAME=wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
WCS-calibrated image found: wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
Checking if the catalog wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
WCS catalog name: wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.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=373, bad_region=817, passed=5521
Got 5521 stars (including 4367 good ones) from the SExtractor catalog wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits.wcscat
util/solve_plate_with_UCAC5 got 5521 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.7'
Seting catalog search parameters based on the expected field of view 940.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013065 (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 0.010452 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 4738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 4738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 4738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 927 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits N_match=927 sigma_overall_arcsec=0.536 sigma_q1_arcsec=0.538 sigma_q2_arcsec=0.446 sigma_q3_arcsec=0.646 sigma_q4_arcsec=0.495 n_q1=284 n_q2=149 n_q3=349 n_q4=145 worst_quadrant_to_overall_ratio=1.206
The image catalog is written to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits -region wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits sigma_overall=0.484 worst_q_ratio=1.214
ref2=Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits sigma_overall=0.471 worst_q_ratio=1.201
new1=fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits sigma_overall=0.551 worst_q_ratio=1.108
new2=fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits sigma_overall=0.536 worst_q_ratio=1.206
reference average sigma_overall=0.4775 worst_q_ratio=1.2075
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056_astrometric_residuals.png (928 matched stars from wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057_astrometric_residuals.png (934 matched stars from wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470_astrometric_residuals.png (929 matched stars from wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471_astrometric_residuals.png (927 matched stars from wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits'
Saving fully-calibrated image wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits'
Preparing the HTML report for the field Aur-06-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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31541_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 31541_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:41:21.55 +29:29:38.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17096_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 17096_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:04:17.04 +28:29:02.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Aur-06-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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
SExtractor catalog cache: saved Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.cat to cache
SExtractor catalog cache: saved Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Creating symlink local_wcs_cache/wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits exists and is non-empty
wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits exists and is non-empty
wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits exists and is non-empty
wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits (1st reference image)
verification OK: wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:00.480 +29:59:52.07 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-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits (1st new image)
verification OK: wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
Image size: 940.7'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 06:00:24.969 +30:02:29.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:00:00.480 +29:59:52.07
Second-epoch image center 06:00:24.969 +30:02:29.56
Angular distance between the image centers 0.0986 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits (2nd new image)
verification OK: wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
Image size: 940.7'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 06:00:28.120 +30:01:50.98 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:00:00.480 +29:59:52.07
Second-epoch image center 06:00:28.120 +30:01:50.98
Angular distance between the image centers 0.1051 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:00:24.969 +30:02:29.56
Second-epoch second image center 06:00:28.120 +30:01:50.98
Angular distance between the image centers 0.01562 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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits &> /tmp/tmp.sB4GIufVRo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits &> /tmp/tmp.j1rCkfsMqt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits &> /tmp/tmp.DTxRCh3giJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits &> /tmp/tmp.ODBe1bxrUS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits and wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits and wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat
Found non-empty wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits and wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat
The reference image (wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits) and catalog (wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat) found
'wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat' -> 'wcsmag.cat'
Read 212828 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.5608 to 99.6889 deg, Dec +24.3185 to +35.3069 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 80.5608 to 99.6889 deg, Dec 24.3185 to 35.3069 deg
Loaded 17188 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): 9142 out of 14161 total matches.
Matched with Tycho-2 14161 out of 212828 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.778800
a=0.000000 b=1.000000 c=22.778800
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 212828 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.5608 to 99.6889 deg, Dec +24.3185 to +35.3069 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 80.5608 to 99.6889 deg, Dec 24.3185 to 35.3069 deg
Loaded 17188 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): 9142 out of 14161 total matches.
Matched with Tycho-2 14161 out of 212828 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits:
Forced-photometry filter: calibrated wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits -> calib.txt_param_ref_wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits (aperture=4.4)
Read 212641 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 80.5698 to 99.6891 deg, Dec +24.3258 to +35.3145 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 80.5698 to 99.6891 deg, Dec 24.3258 to 35.3145 deg
Loaded 17176 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): 9258 out of 14259 total matches.
Matched with Tycho-2 14259 out of 212641 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits:
Forced-photometry filter: calibrated wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits -> calib.txt_param_ref_wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 62 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
1.9 pix Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
2.2 pix fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
2.2 pix fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
1.9 pix wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
1.9 pix wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
Limiting magnitude estimates:
15.5 mag. Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
15.5 mag. Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
13.5 mag. fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
13.5 mag. fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 13.1 (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.sB4GIufVRo (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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits' -> 'wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
WCS_IMAGE_NAME=wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
WCS-calibrated image found: wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
Checking if the catalog wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat corresponding to the image wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits alredy exist and is non-empty...
Catalog wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat corresponding to the image wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits
WCS catalog name: wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=61, blended=32425, bad_region=34270, passed=212766
Got 212766 stars (including 150203 good ones) from the SExtractor catalog wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat
util/solve_plate_with_UCAC5 got 212766 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 181905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 181905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 181908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits N_match=931 sigma_overall_arcsec=0.485 sigma_q1_arcsec=0.539 sigma_q2_arcsec=0.397 sigma_q3_arcsec=0.468 sigma_q4_arcsec=0.485 n_q1=258 n_q2=185 n_q3=292 n_q4=196 worst_quadrant_to_overall_ratio=1.112
The image catalog is written to wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits -region wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.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.j1rCkfsMqt (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-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits' -> 'wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
WCS-calibrated image found: wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
Checking if the catalog wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat corresponding to the image wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits
WCS catalog name: wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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=36, blended=32176, bad_region=34340, passed=212605
Got 212605 stars (including 150130 good ones) from the SExtractor catalog wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat
util/solve_plate_with_UCAC5 got 212605 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 182100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 182100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 182100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits N_match=937 sigma_overall_arcsec=0.495 sigma_q1_arcsec=0.603 sigma_q2_arcsec=0.435 sigma_q3_arcsec=0.450 sigma_q4_arcsec=0.428 n_q1=265 n_q2=192 n_q3=275 n_q4=205 worst_quadrant_to_overall_ratio=1.218
The image catalog is written to wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits -region wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.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.DTxRCh3giJ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
WCS_IMAGE_NAME=wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
WCS-calibrated image found: wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
Checking if the catalog wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
WCS catalog name: wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.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=5, blended=2605, bad_region=5631, passed=53590
Got 53590 stars (including 45537 good ones) from the SExtractor catalog wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits.wcscat
util/solve_plate_with_UCAC5 got 53590 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.7'
Seting catalog search parameters based on the expected field of view 940.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013065 (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 0.010452 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 48254 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 48255 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 48255 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 924 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits N_match=924 sigma_overall_arcsec=0.563 sigma_q1_arcsec=0.556 sigma_q2_arcsec=0.520 sigma_q3_arcsec=0.640 sigma_q4_arcsec=0.544 n_q1=289 n_q2=154 n_q3=327 n_q4=154 worst_quadrant_to_overall_ratio=1.136
The image catalog is written to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits -region wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.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.ODBe1bxrUS (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
WCS_IMAGE_NAME=wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
WCS-calibrated image found: wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
Checking if the catalog wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits.wcscat corresponding to the image wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
WCS catalog name: wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.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=1, no_mag_err=0, low_SNR=6, blended=2554, bad_region=5398, passed=51824
Got 51824 stars (including 43987 good ones) from the SExtractor catalog wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits.wcscat
util/solve_plate_with_UCAC5 got 51824 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.7'
Seting catalog search parameters based on the expected field of view 940.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013065 (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 0.010452 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 46660 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
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 46661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 46662 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits N_match=926 sigma_overall_arcsec=0.566 sigma_q1_arcsec=0.599 sigma_q2_arcsec=0.454 sigma_q3_arcsec=0.663 sigma_q4_arcsec=0.547 n_q1=296 n_q2=151 n_q3=328 n_q4=151 worst_quadrant_to_overall_ratio=1.171
The image catalog is written to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits -region wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.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-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-41-26_20.00sec_4.90C_LIGHT_0470.fits
Saving fully-calibrated image wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-23_CI_Aur-06-Q2b1x1_063914_TTUQ2b1x1_3698727_E3GboMVC/wcs_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471.fits
Preparing the HTML report for the field Aur-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:52:17.85 +32:30:12.3: 12.90 +/- 0.14 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:01:10.57 +31:44:22.4: 13.41 +/- 0.03 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:45:12.11 +28:09:51.1: 12.40 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:06:32.46 +27:23:00.7: 13.11 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:54:35.37 +31:12:41.1: 13.04 +/- 0.03 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:52:24.95 +32:25:58.7: 11.60 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:01:10.57 +31:44:22.4: 13.39 +/- 0.03 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:06:32.46 +27:23:00.7: 13.05 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:52:17.85 +32:30:12.3: 12.85 +/- 0.13 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:45:12.11 +28:09:51.1: 12.37 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:54:35.37 +31:12:41.1: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry reference-image weighted average: 12.87 +/- 0.10
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter REJECTED candidate at 06:01:10.57 +31:44:22.4: ref_mag=13.40 +/- 0.02 new_mean_mag=13.3933 delta=0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:06:32.46 +27:23:00.7: ref_mag=13.08 +/- 0.02 new_mean_mag=12.9941 delta=0.08 (need > 0.90)
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter REJECTED candidate at 05:52:17.85 +32:30:12.3: ref_mag=12.87 +/- 0.10 new_mean_mag=12.6710 delta=0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:45:12.11 +28:09:51.1: ref_mag=12.39 +/- 0.01 new_mean_mag=12.4931 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:54:35.37 +31:12:41.1: ref_mag=13.05 +/- 0.02 new_mean_mag=12.9862 delta=0.06 (need > 0.90)
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:52:24.95 +32:25:58.7: 11.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Forced photometry filter REJECTED candidate at 05:52:24.95 +32:25:58.7: ref_mag=11.64 +/- 0.01 new_mean_mag=11.9414 delta=-0.30 (need > 0.90)
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:53:00.98 +33:33:30.3: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:53:00.98 +33:33:30.3: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:09:50.69 +31:24:42.8: 12.63 +/- 0.02 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:44:49.57 +30:37:23.5: 13.01 +/- 0.03 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 06:16:17.54 +33:40:01.7: 12.46 +/- 0.01 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:09:50.69 +31:24:42.8: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter REJECTED candidate at 06:09:50.69 +31:24:42.8: ref_mag=12.65 +/- 0.01 new_mean_mag=12.5353 delta=0.12 (need > 0.90)
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:44:49.57 +30:37:23.5: 13.04 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 06:16:17.54 +33:40:01.7: 12.48 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 05:44:49.57 +30:37:23.5: ref_mag=13.03 +/- 0.02 new_mean_mag=12.7804 delta=0.25 (need > 0.90)
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter REJECTED candidate at 06:16:17.54 +33:40:01.7: ref_mag=12.47 +/- 0.01 new_mean_mag=12.6016 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:53:52.92 +26:15:26.5: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:53:52.92 +26:15:26.5: 15.83 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.83 +/- 0.27
Forced photometry filter KEPT candidate at 05:53:52.92 +26:15:26.5: ref_mag=15.83 +/- 0.27 new_mean_mag=12.7437 delta=3.09 (need > 0.90)
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-52-31_20.00sec_-15.00C_LIGHT_0056.fits at 05:46:15.94 +31:13:33.6: 13.31 +/- 0.03 detection
Forced photometry on wcs_Aur-06-Q2b1x1_2026-02-21_20-53-39_20.00sec_-14.90C_LIGHT_0057.fits at 05:46:15.94 +31:13:33.6: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter KEPT candidate at 05:46:15.94 +31:13:33.6: ref_mag=13.34 +/- 0.02 new_mean_mag=12.2083 delta=1.13 (need > 0.90)
Adding exclusion_list_local.txt__out242010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80109.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 239231_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239231_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
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Considering the candidate 239235_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239235_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:47:46.82 +29:05:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239238_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239238_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
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Considering the candidate 239242_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239242_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
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Considering the candidate 239253_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239253_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:47:58.84 +32:18:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239255_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239255_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:07:38.47 +29:55:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239258_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239258_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:04:28.95 +27:18:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239263_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239263_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
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Considering the candidate 239269_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239269_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
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Considering the candidate 239270_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239270_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:41:11.93 +26:16:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239271_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239271_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:53:00.82 +27:35:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239274_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239274_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:56:33.27 +29:54:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239279_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239279_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
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Considering the candidate 239281_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239281_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:55:59.27 +30:27:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239282_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239282_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:52:14.61 +32:34:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239283_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239283_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:52:18.04 +32:31:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239284_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239284_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:52:07.70 +32:34:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239285_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 239285_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:41:21.57 +29:29:38.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 241042_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 241042_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:42:12.27 +32:03:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242010_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
Preparing report for the candidate 242010_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
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Considering the candidate 242186_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 242186_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:52:16.27 +32:35:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242381_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 242381_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:51:00.40 +27:56:29.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 242721_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 242721_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:00:52.64 +27:35:11.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 242829_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 242829_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:09:27.62 +28:29:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243404_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 243404_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:58:01.89 +25:55:16.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 244112_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 244112_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:52:23.32 +28:38:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244231_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 244231_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:12:10.40 +32:41:29.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 244485_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 244485_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:52:11.64 +32:30:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244642_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 244642_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:07:02.54 +26:39:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244976_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 244976_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:58:51.92 +29:59:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245307_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 245307_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:14:05.75 +33:13:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245378_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 245378_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:06:18.77 +29:32:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245504_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 245504_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:40:55.11 +32:52:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245738_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 245738_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
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Considering the candidate 245831_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 245831_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:39:20.85 +30:53:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246041_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 246041_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
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Considering the candidate 246200_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 246200_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:40:45.40 +27:47:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246271_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 246271_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:06:56.92 +26:41:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246312_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 246312_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
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Considering the candidate 246324_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 246324_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:03:15.59 +31:22:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246359_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 246359_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:01:20.69 +32:38:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246543_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 246543_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:06:15.93 +32:18:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246918_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 246918_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:05:03.58 +26:04:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247144_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 247144_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:44:34.72 +30:30:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247435_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 247435_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:52:24.61 +28:37:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247471_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 247471_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:51:15.13 +32:06:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247884_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 247884_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:11:48.46 +31:10:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247958_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
Preparing report for the candidate 247958_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
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Considering the candidate 248108_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 248108_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:55:55.28 +28:47:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248337_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 248337_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:08:31.97 +27:49:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249978_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 249978_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:45:50.89 +30:45:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250048_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 250048_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:03:27.27 +27:37:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250308_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 250308_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:42:13.45 +32:04:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80109_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
Preparing report for the candidate 80109_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
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Considering the candidate 115105_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 115105_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:49:47.46 +29:32:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137469_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 137469_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:04:16.95 +28:29:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107520_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 107520_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:04:28.63 +29:51:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 63229_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 63229_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:48:03.16 +32:03:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56703_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 56703_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:57:14.70 +32:22:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156560_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 156560_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 05:40:49.23 +27:36:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158400_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 158400_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 06:15:28.29 +27:23:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 88249_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471
The candidate 88249_fd_Aur-06-Q2b1x1_2026-07-23_05-42-15_20.00sec_4.90C_LIGHT_0471 did not pass the final checks