This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB
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 09 03.1951 2461286.6951 9.77 04:15:39.99 +49:18:58.9
153.40322 -1.08177 galactic Per Second-epoch detections are separated by 0.4" and 3.4 pix
The object was found in VSX 2" V1028 Per
Type: LB
# Max. Min./Amp. JD0 Period
9.350 R1 10.000 R1
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 04:15:39.99 +49:18:58.9: 10.70 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:15:39.99 +49:18:58.9: 10.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.70 +/- 0.00
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 09 03.1951* 04 15 39.99 +49 18 58.9 9.8 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
V1028 Per,2461286.6951,9.77,0.05,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
V1028 Per 20260903.1951 9.77CV 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 09 03.1951* 03 31 12.01 +43 54 15.3 11.3 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,2461286.6951,11.32,0.05,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 20260903.1951 11.32CV 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 09 03.1951 2461286.6951 11.96 04:07:45.99 +43:32:48.6
156.36395 -6.22074 galactic Per Second-epoch detections are separated by 1.2" and 3.2 pix
The object was found in VSX 1" ASASSN-V J040746.09+433248.0
Type: L
# Max. Min./Amp. JD0 Period
13.470 V 13.920 V
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 04:07:45.99 +43:32:48.6: 12.85 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:07:45.99 +43:32:48.6: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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 09 03.1951* 04 07 45.99 +43 32 48.6 12.0 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
ASASSN-V J040746.09+433248.0,2461286.6951,11.96,0.05,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
ASASSN-V J040746.09+433248.0 20260903.1951 11.96CV 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
## 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: 2461286.69532671 03.09.2026 04:41:06.228 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 6 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): 23305
Objects passed selection criteria: 23140
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: 14398.5
Average stars matched: 13907.2 (96.5882 %)
Memory usage VmPeak: 247840 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 3 00:52:40 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: 2461286.69532671 03.09.2026 04:41:06.228 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 90
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: 38 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): 172365
Objects passed selection criteria: 171707
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: 109342
Average stars matched: 104932 (95.9672 %)
Memory usage VmPeak: 569116 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 3 00:54:21 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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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: 2461286.69480753
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
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_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits exists and is non-empty
wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits (1st new image)
verification OK: wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.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: 03:36:08.086 +45:54:33.76 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 03:36:08.086 +45:54:33.76
Angular distance between the image centers 0.0925 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits (2nd new image)
verification OK: wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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: 03:36:10.174 +45:54:29.29 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 03:36:10.174 +45:54:29.29
Angular distance between the image centers 0.0951 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 03:36:08.086 +45:54:33.76
Second-epoch second image center 03:36:10.174 +45:54:29.29
Angular distance between the image centers 0.00618 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.ctyi26y2cl
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.WTw2lEHTey
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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits &> /tmp/tmp.nMdAe70Vb4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits &> /tmp/tmp.s4Vy9R4Pai
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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 3 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
2.9 pix fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
2.9 pix fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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
12.7 mag. fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
12.6 mag. fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 10.5 (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
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.ctyi26y2cl (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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/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
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.WTw2lEHTey (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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/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
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.nMdAe70Vb4 (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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
WCS-calibrated image found: wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
Checking if the catalog wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.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_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
WCS catalog name: wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.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=175, bad_region=0, passed=3988
Got 3988 stars (including 3808 good ones) from the SExtractor catalog wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat
util/solve_plate_with_UCAC5 got 3988 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 650 to 708 (Dec 40.1 to 51.2)
Done reading UCAC5 zone files...
Matched 3733 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3704 matched stars entering correct_measured_positions(), 3703 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3704 matched stars entering correct_measured_positions(), 3987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 650 to 708 (Dec 40.1 to 51.2)
Done reading UCAC5 zone files...
Matched 3732 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3704 matched stars entering correct_measured_positions(), 3987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 3704 matched stars entering correct_measured_positions(), 3987 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 3704 stars left (next iteration limit 4074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3704 robust_rms=7.490 arcsec worst_quadrant_rms=31.239 arcsec
SIP_REFIT: SIP order 3 trial: matched=3704 robust_rms=0.599 arcsec worst_quadrant_rms=0.893 arcsec
SIP_REFIT: SIP order 5 trial: matched=3704 robust_rms=0.490 arcsec worst_quadrant_rms=0.604 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3704 robust_rms_before=1.518 arcsec robust_rms_before_corrected=0.480 arcsec robust_rms_after=0.490 arcsec worst_quadrant_rms_before=0.626 worst_quadrant_rms_after=0.604
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.626 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits N_match=3704 sigma_overall_arcsec=0.480 sigma_q1_arcsec=0.485 sigma_q2_arcsec=0.632 sigma_q3_arcsec=0.386 sigma_q4_arcsec=0.510 n_q1=1248 n_q2=543 n_q3=1106 n_q4=807 worst_quadrant_to_overall_ratio=1.315
The image catalog is written to wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits -region wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.s4Vy9R4Pai (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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
WCS-calibrated image found: wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
Checking if the catalog wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
WCS catalog name: wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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=191, bad_region=0, passed=3998
Got 3998 stars (including 3804 good ones) from the SExtractor catalog wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat
util/solve_plate_with_UCAC5 got 3998 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 650 to 708 (Dec 40.0 to 51.2)
Done reading UCAC5 zone files...
Matched 3745 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3721 matched stars entering correct_measured_positions(), 3722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3721 matched stars entering correct_measured_positions(), 3998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 650 to 708 (Dec 40.0 to 51.2)
Done reading UCAC5 zone files...
Matched 3744 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3722 matched stars entering correct_measured_positions(), 3998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 3722 matched stars entering correct_measured_positions(), 3998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 3722 stars left (next iteration limit 4093)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3722 robust_rms=7.527 arcsec worst_quadrant_rms=26.400 arcsec
SIP_REFIT: SIP order 3 trial: matched=3722 robust_rms=0.627 arcsec worst_quadrant_rms=0.953 arcsec
SIP_REFIT: SIP order 5 trial: matched=3722 robust_rms=0.494 arcsec worst_quadrant_rms=0.657 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3722 robust_rms_before=1.468 arcsec robust_rms_before_corrected=0.492 arcsec robust_rms_after=0.494 arcsec worst_quadrant_rms_before=0.678 worst_quadrant_rms_after=0.657
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.678 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits N_match=3722 sigma_overall_arcsec=0.482 sigma_q1_arcsec=0.497 sigma_q2_arcsec=0.691 sigma_q3_arcsec=0.383 sigma_q4_arcsec=0.480 n_q1=1260 n_q2=540 n_q3=1099 n_q4=823 worst_quadrant_to_overall_ratio=1.433
The image catalog is written to wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits -region wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) 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'
Saving the final (post-refit) 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'
Saving the final (post-refit) wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits to local_wcs_cache/
'wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits' -> 'local_wcs_cache/wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits'
Saving the final (post-refit) wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits to local_wcs_cache/
'wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits' -> 'local_wcs_cache/wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits'
###################################
# 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_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits sigma_overall=0.480 worst_q_ratio=1.315
new2=fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits sigma_overall=0.482 worst_q_ratio=1.433
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_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121_astrometric_residuals.png (3704 matched stars from wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122_astrometric_residuals.png (3722 matched stars from wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.45 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits'
Saving fully-calibrated image wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits'
Preparing the HTML report for the field Per-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 04:15:39.99 +49:18:58.9: 10.70 +/- 0.00 detection
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:15:39.99 +49:18:58.9: 10.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.70 +/- 0.00
Forced photometry filter KEPT candidate at 04:15:39.99 +49:18:58.9: ref_mag=10.70 +/- 0.00 new_mean_mag=9.7696 delta=0.93 (need > 0.90)
Adding exclusion_list_local.txt__out19804.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04594_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 04594_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:09:34.43 +42:19:47.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08393_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 08393_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:29:23.36 +44:24:26.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19804_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
Preparing report for the candidate 19804_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
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 ####
04:15:39.99 +49:18:58.9
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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
Creating symlink local_wcs_cache/wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
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_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits exists and is non-empty
wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits (1st new image)
verification OK: wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.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: 03:36:08.086 +45:54:33.76 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 03:36:08.086 +45:54:33.76
Angular distance between the image centers 0.0925 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits (2nd new image)
verification OK: wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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: 03:36:10.174 +45:54:29.29 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 03:36:10.174 +45:54:29.29
Angular distance between the image centers 0.0951 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 03:36:08.086 +45:54:33.76
Second-epoch second image center 03:36:10.174 +45:54:29.29
Angular distance between the image centers 0.00618 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.FsKaVXocvH
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.qKTkLmorsC
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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits &> /tmp/tmp.tb3MhpKIJZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits &> /tmp/tmp.4XFlgSnhOk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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 83 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
2.8 pix fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
2.7 pix fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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
13.2 mag. fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
13.2 mag. fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.7 (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.FsKaVXocvH (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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/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 - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
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=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
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.qKTkLmorsC (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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/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 - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
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=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
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.tb3MhpKIJZ (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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
WCS-calibrated image found: wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
Checking if the catalog wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.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_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
WCS catalog name: wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.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=1, no_mag_err=0, low_SNR=3, blended=956, bad_region=1, passed=31157
Got 31157 stars (including 30145 good ones) from the SExtractor catalog wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat
util/solve_plate_with_UCAC5 got 31157 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 649 to 708 (Dec 40.0 to 51.3)
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(), 4872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 31157 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 4907 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(), 31157 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 31157 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4874 robust_rms=6.716 arcsec worst_quadrant_rms=39.483 arcsec
SIP_REFIT: SIP order 3 trial: matched=4874 robust_rms=0.611 arcsec worst_quadrant_rms=0.883 arcsec
SIP_REFIT: SIP order 5 trial: matched=4874 robust_rms=0.505 arcsec worst_quadrant_rms=0.639 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4874 robust_rms_before=1.528 arcsec robust_rms_before_corrected=0.473 arcsec robust_rms_after=0.505 arcsec worst_quadrant_rms_before=0.623 worst_quadrant_rms_after=0.639
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.623 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits N_match=4874 sigma_overall_arcsec=0.467 sigma_q1_arcsec=0.476 sigma_q2_arcsec=0.615 sigma_q3_arcsec=0.388 sigma_q4_arcsec=0.503 n_q1=1630 n_q2=702 n_q3=1535 n_q4=1007 worst_quadrant_to_overall_ratio=1.319
The image catalog is written to wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits -region wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.4XFlgSnhOk (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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
WCS-calibrated image found: wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
Checking if the catalog wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat corresponding to the image wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits
WCS catalog name: wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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=993, bad_region=3, passed=31579
Got 31579 stars (including 30533 good ones) from the SExtractor catalog wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat
util/solve_plate_with_UCAC5 got 31579 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 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 4892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 31579 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 31579 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 31579 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4893 stars left (next iteration limit 5381)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4893 robust_rms=6.747 arcsec worst_quadrant_rms=32.167 arcsec
SIP_REFIT: SIP order 3 trial: matched=4893 robust_rms=0.628 arcsec worst_quadrant_rms=0.938 arcsec
SIP_REFIT: SIP order 5 trial: matched=4893 robust_rms=0.499 arcsec worst_quadrant_rms=0.662 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4893 robust_rms_before=1.480 arcsec robust_rms_before_corrected=0.465 arcsec robust_rms_after=0.499 arcsec worst_quadrant_rms_before=0.655 worst_quadrant_rms_after=0.662
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.655 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits N_match=4893 sigma_overall_arcsec=0.461 sigma_q1_arcsec=0.470 sigma_q2_arcsec=0.651 sigma_q3_arcsec=0.381 sigma_q4_arcsec=0.480 n_q1=1606 n_q2=704 n_q3=1534 n_q4=1049 worst_quadrant_to_overall_ratio=1.411
The image catalog is written to wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits -region wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/wcs_fd_Per-02-Q1b1x1_2026-09-02_23-40-21_20.00sec_-0.00C_LIGHTs_0121.fits
Saving fully-calibrated image wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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_2026-09-03_CI_Per-02-Q1b1x1_004816_TTUQ1b1x1_2400081_BD9YQMeB/wcs_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122.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 04:07:45.99 +43:32:48.6: 12.85 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q1b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 04:07:45.99 +43:32:48.6: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter KEPT candidate at 04:07:45.99 +43:32:48.6: ref_mag=12.85 +/- 0.01 new_mean_mag=11.9418 delta=0.90 (need > 0.90)
Adding exclusion_list_local.txt__out44462.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215053_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215053_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 02:54:03.65 +45:53:18.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215057_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215057_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:21:33.30 +46:29:53.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215059_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215059_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 02:54:14.62 +42:35:17.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215123_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215123_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215230_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215230_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215269_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215269_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215285_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215285_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 02:59:33.21 +41:00:55.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215389_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215389_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:09:13.89 +44:50:34.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215419_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215419_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:53:30.16 +47:39:02.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215538_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215538_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215614_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215614_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215652_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215652_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 02:55:34.26 +48:21:27.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215767_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215767_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:51:30.27 +45:27:31.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215768_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215768_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215838_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215838_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:07:58.37 +40:54:32.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215846_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215846_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215867_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215867_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215888_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215888_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:44:45.09 +46:07:13.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215925_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215925_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215959_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 215959_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 02:56:38.23 +47:11:09.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216011_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 216011_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:56:43.22 +50:40:44.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216056_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 216056_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216099_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 216099_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:17:45.83 +43:59:59.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216124_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 216124_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 02:59:47.05 +47:14:55.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216130_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 216130_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216183_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 216183_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:46:04.39 +45:42:23.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216219_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 216219_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 02:57:48.38 +46:39:04.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216266_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 216266_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:11:59.47 +46:06:26.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165306_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 165306_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:06:34.83 +50:21:01.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15977_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 15977_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:08:10.26 +40:57:19.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66312_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 66312_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:29:23.37 +44:24:26.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117836_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 117836_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:50:56.28 +47:14:35.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179416_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 179416_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 145807_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 145807_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:54:56.78 +48:36:02.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201737_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 201737_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:18:27.92 +42:49:18.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57693_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 57693_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:20:22.20 +43:51:20.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48255_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 48255_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:37:25.10 +43:39:08.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51608_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 51608_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:15:49.77 +43:25:05.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31744_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 31744_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:30:56.31 +42:37:24.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16835_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 16835_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:56:15.66 +41:59:29.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125439_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 125439_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:53:37.43 +47:38:52.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185018_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 185018_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:05:22.72 +49:11:57.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20258_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 20258_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:04:06.80 +42:12:13.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54778_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
Preparing report for the candidate 54778_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33246_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 33246_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:14:44.10 +42:22:53.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17732_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 17732_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:00:20.82 +42:02:58.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52293_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 52293_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:12:15.70 +43:20:09.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44462_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
Preparing report for the candidate 44462_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143151_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 143151_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 02:57:56.73 +47:45:35.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105098_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 105098_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:04:33.91 +46:36:39.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175405_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 175405_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:21:34.75 +49:37:13.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138067_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 138067_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:12:05.08 +48:13:54.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82973_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 82973_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:49:29.55 +45:29:52.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51743_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 51743_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:49:26.56 +43:54:08.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64075_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 64075_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:01:21.91 +44:36:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53524_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 53524_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:23:35.25 +43:39:31.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132584_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 132584_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:16:06.56 +47:54:48.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33764_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 33764_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:48:45.52 +42:55:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21493_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 21493_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:07:57.37 +42:13:20.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36093_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 36093_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:09:34.44 +42:19:47.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181609_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 181609_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:15:39.98 +49:18:58.8 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83744_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 83744_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:04:17.19 +45:25:39.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100381_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 100381_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:32:26.20 +46:03:19.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 97528_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 97528_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:44:40.74 +46:05:56.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89159_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 89159_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:45:59.11 +45:40:52.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67567_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 67567_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:28:18.33 +44:22:38.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133414_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 133414_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:42:55.41 +47:47:08.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170155_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 170155_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:36:29.40 +48:11:27.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74335_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 74335_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:50:04.13 +44:58:02.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138730_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 138730_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:30:34.59 +47:59:39.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 145961_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 145961_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:44:06.40 +48:31:22.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54036_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 54036_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:49:07.94 +43:57:47.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30459_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 30459_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:45:11.48 +42:34:45.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131725_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 131725_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:55:58.00 +47:52:13.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64602_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 64602_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:17:47.71 +44:01:29.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50351_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 50351_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:21:26.75 +43:19:48.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185390_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 185390_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:53:38.65 +48:38:59.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139144_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 139144_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:24:19.62 +49:51:33.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86613_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 86613_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:09:30.62 +44:51:22.7 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169063_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 169063_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:19:13.41 +50:02:54.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160280_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 160280_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 03:56:36.70 +50:41:38.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130730_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 130730_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks
**** FOUND 04:08:39.42 +47:42:41.6 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147078_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122
The candidate 147078_fd_Per-02-Q1b1x1_2026-09-02_23-41-06_20.00sec_0.00C_LIGHTs_0122 did not pass the final checks