This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 06.2707 2461258.7707 12.86 03:31:37.34 +47:45:31.0
148.76198 -6.91754 galactic Per Second-epoch detections are separated by 1.5" and 6.8 pix
The object was found in VSX 0" NSVS 4123600
Type: SR|L
# Max. Min./Amp. JD0 Period
12.063 R1 12.847 R1 2451482.09000 111.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:31:37.34 +47:45:31.0: 13.95 +/- 0.04 detection
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:31:37.34 +47:45:31.0: 13.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2707* 03 31 37.34 +47 45 31.0 12.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 4123600,2461258.7707,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 4123600 20260806.2707 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2707 2461258.7707 12.48 03:42:21.49 +48:04:05.0
150.03631 -5.60338 galactic Per Second-epoch detections are separated by 1.4" and 6.4 pix
The object was found in VSX 1" ASASSN-V J034221.54+480404.1
Type: SR
# Max. Min./Amp. JD0 Period
13.820 V 14.310 V 2458490.57110 56.384961100000
The object was not found in astcheck.
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:21.49 +48:04:05.0: 13.47 +/- 0.03 detection
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:21.49 +48:04:05.0: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2707* 03 42 21.49 +48 04 05.0 12.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J034221.54+480404.1,2461258.7707,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J034221.54+480404.1 20260806.2707 12.48CV 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
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 08 06.2707* 03 31 11.99 +43 54 14.9 11.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GK Per,2461258.7707,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GK Per 20260806.2707 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.2707 2461258.7707 11.80 03:44:53.57 +42:22:42.1
153.91379 -9.82408 galactic Per Second-epoch detections are separated by 2.0" and 6.2 pix
The object was found in VSX 2" ASASSN-V J034453.40+422241.7
Type: SR
# Max. Min./Amp. JD0 Period
12.910 V 13.250 V 2457061.80000 45.960000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:44:53.57 +42:22:42.1: 12.84 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:44:53.57 +42:22:42.1: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 06.2707* 03 44 53.57 +42 22 42.1 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J034453.40+422241.7,2461258.7707,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J034453.40+422241.7 20260806.2707 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.58214624 09.01.2026 01:58:07.435 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
First image: 2461049.58214624 09.01.2026 01:58:07.435 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Last image: 2461258.77095816 06.08.2026 06:30:00.785 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 23176
Objects passed selection criteria: 22996
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 13607.5
Average stars matched: 13159 (96.704 %)
Memory usage VmPeak: 248004 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 01:43:02 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: 2461049.58214624 09.01.2026 01:58:07.435 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
First image: 2461049.58214624 09.01.2026 01:58:07.435 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Last image: 2461258.77095816 06.08.2026 06:30:00.785 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 60
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.23
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 28 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 171431
Objects passed selection criteria: 170734
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: 104944
Average stars matched: 100826 (96.076 %)
Memory usage VmPeak: 634648 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 01:44:05 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
SExtractor catalog cache: saved Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.cat to cache
SExtractor catalog cache: saved Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.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/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.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: 2461258.77041681
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_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits exists and is non-empty
Saving wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits to local_wcs_cache/
'wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits' -> 'local_wcs_cache/wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits'
wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits exists and is non-empty
Saving wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits to local_wcs_cache/
'wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits' -> 'local_wcs_cache/wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits'
wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits exists and is non-empty
Saving wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits to local_wcs_cache/
'wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits' -> 'local_wcs_cache/wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits'
wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits exists and is non-empty
Saving wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits to local_wcs_cache/
'wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits' -> 'local_wcs_cache/wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (1st reference image)
verification OK: wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:36:01.913 +46:00:00.61 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits (1st new image)
verification OK: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
Image size: 944.8'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:35:56.762 +46:00:44.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:36:01.913 +46:00:00.61
Second-epoch image center 03:35:56.762 +46:00:44.53
Angular distance between the image centers 0.0193 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits (2nd new image)
verification OK: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
Image size: 944.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:35:56.293 +46:00:05.35 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:36:01.913 +46:00:00.61
Second-epoch image center 03:35:56.293 +46:00:05.35
Angular distance between the image centers 0.0163 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 03:35:56.762 +46:00:44.53
Second-epoch second image center 03:35:56.293 +46:00:05.35
Angular distance between the image centers 0.01097 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/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits &> /tmp/tmp.5EXlhRDQcj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits &> /tmp/tmp.01whyDRp7Y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits &> /tmp/tmp.xO1Xp4k0WX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits &> /tmp/tmp.XCGGlkNOxE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
Found non-empty wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
The reference image (wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits) and catalog (wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat) found
'wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat' -> 'wcsmag.cat'
Read 24919 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2386 to 65.8886 deg, Dec +39.8263 to +51.4097 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 41.2386 to 65.8886 deg, Dec 39.8263 to 51.4097 deg
Loaded 12587 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): 8299 out of 9376 total matches.
Matched with Tycho-2 9376 out of 24919 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.961300
a=0.000000 b=1.000000 c=22.961300
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 24919 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2386 to 65.8886 deg, Dec +39.8263 to +51.4097 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 41.2386 to 65.8886 deg, Dec 39.8263 to 51.4097 deg
Loaded 12587 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): 8299 out of 9376 total matches.
Matched with Tycho-2 9376 out of 24919 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Forced-photometry filter: calibrated wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits -> calib.txt_param_ref_wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (aperture=5.8)
Read 25014 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2390 to 65.8888 deg, Dec +39.8264 to +51.4150 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 41.2390 to 65.8888 deg, Dec 39.8264 to 51.4150 deg
Loaded 12591 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): 8306 out of 9365 total matches.
Matched with Tycho-2 9365 out of 25014 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Forced-photometry filter: calibrated wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits -> calib.txt_param_ref_wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits (aperture=5.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
2.0 pix Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
2.5 pix fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
2.6 pix fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
Limiting magnitude estimates:
15.4 mag. Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
15.4 mag. Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
12.1 mag. fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
12.1 mag. fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
All-image limiting magnitude estimate: 12.1 (SNR ) 10.2 (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.5EXlhRDQcj (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits' -> 'wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Checking if the catalog wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat corresponding to the image wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat corresponding to the image wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS catalog name: wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2608, bad_region=0, passed=24919
Got 24919 stars (including 22273 good ones) from the SExtractor catalog wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
util/solve_plate_with_UCAC5 got 24919 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 4916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 24919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4917 matched stars entering correct_measured_positions(), 24919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4917 matched stars entering correct_measured_positions(), 24919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4917 stars left (next iteration limit 5407)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits N_match=4917 sigma_overall_arcsec=0.415 sigma_q1_arcsec=0.553 sigma_q2_arcsec=0.385 sigma_q3_arcsec=0.375 sigma_q4_arcsec=0.356 n_q1=1270 n_q2=1090 n_q3=1297 n_q4=1260 worst_quadrant_to_overall_ratio=1.334
The image catalog is written to wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits -region wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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.01whyDRp7Y (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits' -> 'wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Checking if the catalog wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat corresponding to the image wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat corresponding to the image wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS catalog name: wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=17, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2561, bad_region=1, passed=24997
Got 24997 stars (including 22411 good ones) from the SExtractor catalog wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat
util/solve_plate_with_UCAC5 got 24997 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4914 matched stars entering correct_measured_positions(), 4914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4914 matched stars entering correct_measured_positions(), 24997 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4915 matched stars entering correct_measured_positions(), 24997 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4915 matched stars entering correct_measured_positions(), 24997 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4915 stars left (next iteration limit 5405)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits N_match=4915 sigma_overall_arcsec=0.389 sigma_q1_arcsec=0.473 sigma_q2_arcsec=0.380 sigma_q3_arcsec=0.359 sigma_q4_arcsec=0.340 n_q1=1272 n_q2=1082 n_q3=1307 n_q4=1254 worst_quadrant_to_overall_ratio=1.218
The image catalog is written to wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits -region wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.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.xO1Xp4k0WX (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
WCS-calibrated image found: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
Checking if the catalog wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
WCS catalog name: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=101, bad_region=0, passed=2394
Got 2394 stars (including 2290 good ones) from the SExtractor catalog wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat
util/solve_plate_with_UCAC5 got 2394 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.8'
Seting catalog search parameters based on the expected field of view 944.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013122 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010498 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 2244 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2222 matched stars entering correct_measured_positions(), 2206 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2222 matched stars entering correct_measured_positions(), 2377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 2244 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2222 matched stars entering correct_measured_positions(), 2376 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 2222 matched stars entering correct_measured_positions(), 2376 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 2222 stars left (next iteration limit 2444)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2222 robust_rms=4.736 arcsec worst_quadrant_rms=6.785 arcsec
SIP_REFIT: SIP order 3 trial: matched=2222 robust_rms=0.500 arcsec worst_quadrant_rms=0.638 arcsec
SIP_REFIT: SIP order 5 trial: matched=2222 robust_rms=0.369 arcsec worst_quadrant_rms=0.408 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2222 robust_rms_before=1.291 arcsec robust_rms_before_corrected=0.410 arcsec robust_rms_after=0.369 arcsec worst_quadrant_rms_before=0.503 worst_quadrant_rms_after=0.408
verification OK: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
verification OK: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
Image size: 945.3'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:35:56.875 +46:00:43.15 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 2394 stars ###
'wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/correct_sextractor_wcs_catalog_usingxy2sky43698.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.291 -> 0.369 arcsec)
WCS_QUALITY_DIAG: file=fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits N_match=2222 sigma_overall_arcsec=0.392 sigma_q1_arcsec=0.439 sigma_q2_arcsec=0.447 sigma_q3_arcsec=0.321 sigma_q4_arcsec=0.365 n_q1=619 n_q2=409 n_q3=460 n_q4=734 worst_quadrant_to_overall_ratio=1.140
The image catalog is written to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits -region wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.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.XCGGlkNOxE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
WCS-calibrated image found: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
Checking if the catalog wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
WCS catalog name: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=104, bad_region=0, passed=2419
Got 2419 stars (including 2311 good ones) from the SExtractor catalog wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat
util/solve_plate_with_UCAC5 got 2419 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.7'
Seting catalog search parameters based on the expected field of view 944.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013121 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010497 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 2265 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2242 matched stars entering correct_measured_positions(), 2217 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2242 matched stars entering correct_measured_positions(), 2393 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 2265 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2243 matched stars entering correct_measured_positions(), 2395 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 2243 matched stars entering correct_measured_positions(), 2395 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 2243 stars left (next iteration limit 2466)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2243 robust_rms=4.716 arcsec worst_quadrant_rms=6.313 arcsec
SIP_REFIT: SIP order 3 trial: matched=2243 robust_rms=0.537 arcsec worst_quadrant_rms=0.690 arcsec
SIP_REFIT: SIP order 5 trial: matched=2243 robust_rms=0.375 arcsec worst_quadrant_rms=0.437 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2243 robust_rms_before=1.350 arcsec robust_rms_before_corrected=0.434 arcsec robust_rms_after=0.375 arcsec worst_quadrant_rms_before=0.515 worst_quadrant_rms_after=0.437
verification OK: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
verification OK: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
Image size: 945.2'x626.8' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:35:56.414 +46:00:03.87 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 2419 stars ###
'wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/correct_sextractor_wcs_catalog_usingxy2sky43699.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.350 -> 0.375 arcsec)
WCS_QUALITY_DIAG: file=fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits N_match=2243 sigma_overall_arcsec=0.407 sigma_q1_arcsec=0.420 sigma_q2_arcsec=0.465 sigma_q3_arcsec=0.346 sigma_q4_arcsec=0.387 n_q1=624 n_q2=422 n_q3=455 n_q4=742 worst_quadrant_to_overall_ratio=1.143
The image catalog is written to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits -region wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.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=Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits sigma_overall=0.415 worst_q_ratio=1.334
ref2=Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits sigma_overall=0.389 worst_q_ratio=1.218
new1=fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits sigma_overall=0.392 worst_q_ratio=1.140
new2=fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits sigma_overall=0.407 worst_q_ratio=1.143
reference average sigma_overall=0.402 worst_q_ratio=1.276
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020_astrometric_residuals.png (4917 matched stars from wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021_astrometric_residuals.png (4915 matched stars from wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218_astrometric_residuals.png (2222 matched stars from wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219_astrometric_residuals.png (2243 matched stars from wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits'
Saving fully-calibrated image wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits'
Preparing the HTML report for the field Per-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Per-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
SExtractor catalog cache: saved Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.cat to cache
SExtractor catalog cache: saved Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Creating symlink local_wcs_cache/wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Creating symlink local_wcs_cache/wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
Creating symlink local_wcs_cache/wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.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_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits exists and is non-empty
wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits exists and is non-empty
wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits exists and is non-empty
wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (1st reference image)
verification OK: wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:36:01.913 +46:00:00.61 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits (1st new image)
verification OK: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
Image size: 944.8'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:35:56.762 +46:00:44.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:36:01.913 +46:00:00.61
Second-epoch image center 03:35:56.762 +46:00:44.53
Angular distance between the image centers 0.0193 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits (2nd new image)
verification OK: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
Image size: 944.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:35:56.293 +46:00:05.35 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:36:01.913 +46:00:00.61
Second-epoch image center 03:35:56.293 +46:00:05.35
Angular distance between the image centers 0.0163 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 03:35:56.762 +46:00:44.53
Second-epoch second image center 03:35:56.293 +46:00:05.35
Angular distance between the image centers 0.01097 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/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits &> /tmp/tmp.MUwzabrAZJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits &> /tmp/tmp.FSazozoxHz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits &> /tmp/tmp.325HGia1ra
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits &> /tmp/tmp.7IoEfM7ioJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
Found non-empty wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
The reference image (wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits) and catalog (wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat) found
'wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat' -> 'wcsmag.cat'
Read 189134 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2226 to 65.9097 deg, Dec +39.7810 to +51.4146 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 41.2226 to 65.9097 deg, Dec 39.7810 to 51.4146 deg
Loaded 12673 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): 6489 out of 9455 total matches.
Matched with Tycho-2 9455 out of 189134 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.834200
a=0.000000 b=1.000000 c=22.834200
From vast_summary.log: estimated ref. image limiting mag.: -7.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.60
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 189134 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2226 to 65.9097 deg, Dec +39.7810 to +51.4146 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 41.2226 to 65.9097 deg, Dec 39.7810 to 51.4146 deg
Loaded 12673 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): 6489 out of 9455 total matches.
Matched with Tycho-2 9455 out of 189134 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Forced-photometry filter: calibrated wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits -> calib.txt_param_ref_wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (aperture=4.4)
Read 187812 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2223 to 65.9102 deg, Dec +39.7810 to +51.4199 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 41.2223 to 65.9102 deg, Dec 39.7810 to 51.4199 deg
Loaded 12677 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): 6500 out of 9428 total matches.
Matched with Tycho-2 9428 out of 187812 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Forced-photometry filter: calibrated wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits -> calib.txt_param_ref_wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 56 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.8 pix Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
1.9 pix Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
2.4 pix fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
2.4 pix fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
Limiting magnitude estimates:
15.6 mag. Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
15.6 mag. Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
13.0 mag. fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
13.0 mag. fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.MUwzabrAZJ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits' -> 'wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Checking if the catalog wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat corresponding to the image wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat corresponding to the image wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS catalog name: wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=52, blended=23506, bad_region=2, passed=189082
Got 189082 stars (including 165266 good ones) from the SExtractor catalog wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
util/solve_plate_with_UCAC5 got 189082 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 4919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 189082 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 189082 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 189082 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4919 stars left (next iteration limit 5410)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits N_match=4919 sigma_overall_arcsec=0.399 sigma_q1_arcsec=0.511 sigma_q2_arcsec=0.387 sigma_q3_arcsec=0.360 sigma_q4_arcsec=0.338 n_q1=1270 n_q2=1122 n_q3=1278 n_q4=1249 worst_quadrant_to_overall_ratio=1.280
The image catalog is written to wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits -region wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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.FSazozoxHz (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits' -> 'wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Checking if the catalog wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat corresponding to the image wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat corresponding to the image wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS catalog name: wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=6, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=57, blended=23390, bad_region=1, passed=187749
Got 187749 stars (including 164063 good ones) from the SExtractor catalog wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat
util/solve_plate_with_UCAC5 got 187749 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 4916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 187749 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 187749 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 187749 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4916 stars left (next iteration limit 5407)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits N_match=4916 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.435 sigma_q2_arcsec=0.379 sigma_q3_arcsec=0.344 sigma_q4_arcsec=0.338 n_q1=1275 n_q2=1106 n_q3=1273 n_q4=1262 worst_quadrant_to_overall_ratio=1.151
The image catalog is written to wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits -region wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.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.325HGia1ra (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
WCS-calibrated image found: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
Checking if the catalog wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
WCS catalog name: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=621, bad_region=1, passed=22371
Got 22371 stars (including 21725 good ones) from the SExtractor catalog wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat
util/solve_plate_with_UCAC5 got 22371 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.8'
Seting catalog search parameters based on the expected field of view 944.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013122 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010498 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.2 to 51.4)
Done reading UCAC5 zone files...
Matched 4915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 4878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 22364 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.2 to 51.4)
Done reading UCAC5 zone files...
Matched 4916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 22364 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 22364 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4880 stars left (next iteration limit 5366)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits N_match=4880 sigma_overall_arcsec=0.459 sigma_q1_arcsec=0.514 sigma_q2_arcsec=0.540 sigma_q3_arcsec=0.370 sigma_q4_arcsec=0.425 n_q1=1345 n_q2=958 n_q3=977 n_q4=1600 worst_quadrant_to_overall_ratio=1.178
The image catalog is written to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits -region wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.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.7IoEfM7ioJ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
WCS-calibrated image found: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
Checking if the catalog wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
WCS catalog name: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=570, bad_region=1, passed=22618
Got 22618 stars (including 22026 good ones) from the SExtractor catalog wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat
util/solve_plate_with_UCAC5 got 22618 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.7'
Seting catalog search parameters based on the expected field of view 944.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013121 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010497 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.2 to 51.4)
Done reading UCAC5 zone files...
Matched 4908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 4869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 22607 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.2 to 51.4)
Done reading UCAC5 zone files...
Matched 4911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 22607 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 22607 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4874 stars left (next iteration limit 5359)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits N_match=4874 sigma_overall_arcsec=0.462 sigma_q1_arcsec=0.478 sigma_q2_arcsec=0.552 sigma_q3_arcsec=0.381 sigma_q4_arcsec=0.436 n_q1=1353 n_q2=967 n_q3=969 n_q4=1585 worst_quadrant_to_overall_ratio=1.194
The image catalog is written to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits -region wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.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_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/wcs_fd_Per-02-Q1b1x1_2026-08-06_01-29-14_20.00sec_-0.00C_LIGHTs_0218.fits
Saving fully-calibrated image wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Per-02-Q1b1x1_013840_TTUQ1b1x1_4101146_7kgI9W7U/wcs_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219.fits
Preparing the HTML report for the field Per-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:33:31.98 +44:04:10.8: 12.44 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:26:54.42 +47:55:29.9: 12.71 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:33:31.98 +44:04:10.8: 12.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter REJECTED candidate at 03:33:31.98 +44:04:10.8: ref_mag=12.44 +/- 0.01 new_mean_mag=12.2213 delta=0.22 (need > 0.90)
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:26:54.42 +47:55:29.9: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry filter REJECTED candidate at 03:26:54.42 +47:55:29.9: ref_mag=12.74 +/- 0.01 new_mean_mag=12.4835 delta=0.25 (need > 0.90)
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:31:37.34 +47:45:31.0: 13.95 +/- 0.04 detection
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:31:37.34 +47:45:31.0: 13.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.03
Forced photometry filter KEPT candidate at 03:31:37.34 +47:45:31.0: ref_mag=13.97 +/- 0.03 new_mean_mag=12.8547 delta=1.12 (need > 0.90)
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:42:21.49 +48:04:05.0: 13.47 +/- 0.03 detection
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:42:21.49 +48:04:05.0: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry filter KEPT candidate at 03:42:21.49 +48:04:05.0: ref_mag=13.45 +/- 0.02 new_mean_mag=12.4472 delta=1.00 (need > 0.90)
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:44:53.57 +42:22:42.1: 12.84 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:44:53.57 +42:22:42.1: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter KEPT candidate at 03:44:53.57 +42:22:42.1: ref_mag=12.81 +/- 0.01 new_mean_mag=11.8062 delta=1.00 (need > 0.90)
Adding exclusion_list_local.txt__out131185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24550.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: 4s
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Considering the candidate 215055_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 215055_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
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Considering the candidate 215060_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 215060_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:24:36.48 +46:21:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215065_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 215065_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 02:54:14.59 +42:35:17.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 215141_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 215141_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:53:30.22 +47:39:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215257_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 215257_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:44:45.10 +46:07:13.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 215270_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 215270_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:30:26.00 +48:06:29.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 215292_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 215292_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:51:30.44 +45:27:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215328_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 215328_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:56:43.21 +50:40:45.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 215378_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 215378_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:09:13.91 +44:50:33.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 215379_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 215379_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 04:03:21.47 +45:45:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215436_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 215436_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:30:43.53 +48:01:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215445_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 215445_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
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Considering the candidate 215447_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 215447_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:31:48.86 +48:45:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50351_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 50351_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:21:26.66 +43:19:49.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 14959_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 14959_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:16:10.39 +41:19:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53524_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 53524_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:23:35.23 +43:39:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51743_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 51743_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:49:26.53 +43:54:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185018_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 185018_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 04:05:22.90 +49:11:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104504_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 104504_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:21:56.85 +46:14:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117836_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 117836_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:50:56.31 +47:14:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131185_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
Preparing report for the candidate 131185_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
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Considering the candidate 175565_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 175565_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:37:08.58 +49:39:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134945_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 134945_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:47:19.29 +48:06:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128521_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 128521_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:26:29.65 +47:31:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100117_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 100117_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:29:49.87 +46:09:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 145807_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 145807_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:54:56.57 +48:36:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201737_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 201737_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:18:27.85 +42:49:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 145271_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 145271_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:39:16.23 +48:35:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55610_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 55610_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:58:00.11 +44:10:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134911_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
Preparing report for the candidate 134911_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
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Considering the candidate 48255_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 48255_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:37:25.03 +43:39:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82031_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 82031_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:30:37.26 +45:15:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31744_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 31744_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:30:56.48 +42:37:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186160_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 186160_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:35:47.22 +49:01:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16835_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 16835_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:56:15.73 +41:59:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89544_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 89544_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:48:27.08 +45:50:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140331_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 140331_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:44:14.92 +48:51:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54778_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
Preparing report for the candidate 54778_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
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Considering the candidate 17732_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 17732_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 04:00:20.91 +42:03:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24550_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
Preparing report for the candidate 24550_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
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Considering the candidate 166395_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 166395_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:42:34.77 +50:15:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138067_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 138067_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 04:12:04.98 +48:13:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82973_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 82973_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:49:29.56 +45:29:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33764_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 33764_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:48:45.49 +42:55:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36093_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 36093_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:09:34.43 +42:19:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92693_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 92693_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
Rejecting candidate due to large distance (36.3") between the two second-epoch detections
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Considering the candidate 66312_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 66312_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:29:23.35 +44:24:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62475_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 62475_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:57:00.52 +44:32:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100381_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 100381_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:32:26.22 +46:03:20.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 133414_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 133414_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:42:55.41 +47:47:09.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 170155_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 170155_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:36:29.42 +48:11:28.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 74335_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 74335_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:50:04.11 +44:58:03.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 30459_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 30459_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 03:45:11.47 +42:34:45.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 165306_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 165306_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 04:06:34.81 +50:21:02.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 130730_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 130730_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks
**** FOUND 04:08:39.39 +47:42:43.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 147078_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219
The candidate 147078_fd_Per-02-Q1b1x1_2026-08-06_01-30-00_20.00sec_-0.00C_LIGHTs_0219 did not pass the final checks