This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT
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 03.3094 2461286.8094 12.64 22:06:25.39 +11:08:29.5
71.08864 -34.63657 galactic Peg Second-epoch detections are separated by 0.8" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.225 Henrietta -0 1 1 12.5 -0 0
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:06:25.39 +11:08:29.5: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:06:25.39 +11:08:29.5: 15.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461286.8094,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260903.3094 12.64CV 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 03.3094 2461286.8094 14.18 22:14:08.99 +09:03:44.9
70.91052 -37.45044 galactic Peg Second-epoch detections are separated by 0.3" and 9.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.105158 2000 OL -0 1 1 14.2 0 0
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:14:08.99 +09:03:44.9: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:14:08.99 +09:03:44.9: 15.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461286.8094,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260903.3094 14.18CV 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: 2461239.82973319 18.07.2026 07:54:38.948 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
First image: 2461239.82973319 18.07.2026 07:54:38.948 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Last image: 2461286.80973573 03.09.2026 07:25:51.167 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 7592
Objects passed selection criteria: 7588
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 6840.5
Average stars matched: 6580.75 (96.2028 %)
Memory usage VmPeak: 233744 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 06:35:03 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: 2461239.82973319 18.07.2026 07:54:38.948 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
First image: 2461239.82973319 18.07.2026 07:54:38.948 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Last image: 2461286.80973573 03.09.2026 07:25:51.167 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 54
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 22 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): 48840
Objects passed selection criteria: 48724
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 45925.5
Average stars matched: 43788.2 (95.3463 %)
Memory usage VmPeak: 270272 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 06:36:16 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/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
SExtractor catalog cache: saved Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.cat to cache
SExtractor catalog cache: saved Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.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/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.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: 2461286.80897747
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_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits exists and is non-empty
wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits exists and is non-empty
wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits exists and is non-empty
wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (1st reference image)
verification OK: wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:09.147 +06:00:12.37 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits (1st new image)
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
Image size: 941.2'x626.7' 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: 22:17:04.617 +06:02:45.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:09.147 +06:00:12.37
Second-epoch image center 22:17:04.617 +06:02:45.83
Angular distance between the image centers 0.0466 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits (2nd new image)
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
Image size: 941.2'x626.7' 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: 22:17:02.090 +06:02:06.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:09.147 +06:00:12.37
Second-epoch image center 22:17:02.090 +06:02:06.34
Angular distance between the image centers 0.0431 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 22:17:04.617 +06:02:45.83
Second-epoch second image center 22:17:02.090 +06:02:06.34
Angular distance between the image centers 0.01516 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/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits &> /tmp/tmp.nXU9RGEvKX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits &> /tmp/tmp.oMRRNbWrbe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits &> /tmp/tmp.ewY2EZnlqN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits &> /tmp/tmp.0JmhcBBO2x
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.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_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.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_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
Found non-empty wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
The reference image (wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits) and catalog (wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat) found
'wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat' -> 'wcsmag.cat'
Read 7642 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.3157 to 342.2143 deg, Dec +0.7081 to +11.2594 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 326.3157 to 342.2143 deg, Dec 0.7081 to 11.2594 deg
Loaded 6032 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): 4873 out of 5003 total matches.
Matched with Tycho-2 5003 out of 7642 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.558200
a=0.000000 b=1.000000 c=22.558200
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.94
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.94
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7642 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.3157 to 342.2143 deg, Dec +0.7081 to +11.2594 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 326.3157 to 342.2143 deg, Dec 0.7081 to 11.2594 deg
Loaded 6032 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): 4873 out of 5003 total matches.
Matched with Tycho-2 5003 out of 7642 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Forced-photometry filter: calibrated wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits -> calib.txt_param_ref_wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (aperture=6.3)
Read 8182 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.3433 to 342.2304 deg, Dec +0.7273 to +11.2580 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 326.3433 to 342.2304 deg, Dec 0.7273 to 11.2580 deg
Loaded 6015 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): 4922 out of 5084 total matches.
Matched with Tycho-2 5084 out of 8182 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Forced-photometry filter: calibrated wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits -> calib.txt_param_ref_wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
2.3 pix Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
2.1 pix fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
2.1 pix fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
Limiting magnitude estimates:
14.9 mag. Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
15.0 mag. Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
14.7 mag. fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
14.7 mag. fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.7 (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.nXU9RGEvKX (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits' -> 'wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.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/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS-calibrated image found: wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Checking if the catalog wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS catalog name: wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.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=416, bad_region=0, passed=7642
Got 7642 stars (including 7221 good ones) from the SExtractor catalog wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 7642 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4564 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4531 matched stars entering correct_measured_positions(), 4531 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4531 matched stars entering correct_measured_positions(), 7642 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4564 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4530 matched stars entering correct_measured_positions(), 7642 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4530 matched stars entering correct_measured_positions(), 7642 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4530 stars left (next iteration limit 4984)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits N_match=4530 sigma_overall_arcsec=0.426 sigma_q1_arcsec=0.352 sigma_q2_arcsec=0.450 sigma_q3_arcsec=0.451 sigma_q4_arcsec=0.461 n_q1=1268 n_q2=894 n_q3=1327 n_q4=1041 worst_quadrant_to_overall_ratio=1.083
The image catalog is written to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits -region wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.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.oMRRNbWrbe (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits' -> 'wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.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/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS-calibrated image found: wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Checking if the catalog wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS catalog name: wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.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=449, bad_region=0, passed=8182
Got 8182 stars (including 7721 good ones) from the SExtractor catalog wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat
util/solve_plate_with_UCAC5 got 8182 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4550 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4515 matched stars entering correct_measured_positions(), 4515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4515 matched stars entering correct_measured_positions(), 8182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4550 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4515 matched stars entering correct_measured_positions(), 8182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4515 matched stars entering correct_measured_positions(), 8182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4515 stars left (next iteration limit 4966)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits N_match=4515 sigma_overall_arcsec=0.464 sigma_q1_arcsec=0.409 sigma_q2_arcsec=0.509 sigma_q3_arcsec=0.432 sigma_q4_arcsec=0.487 n_q1=1053 n_q2=1347 n_q3=888 n_q4=1227 worst_quadrant_to_overall_ratio=1.097
The image catalog is written to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits -region wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.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.ewY2EZnlqN (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_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.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_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
Checking if the catalog wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.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_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
WCS catalog name: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.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=346, bad_region=0, passed=5888
Got 5888 stars (including 5534 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits.wcscat
util/solve_plate_with_UCAC5 got 5888 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.4 to 11.7)
Done reading UCAC5 zone files...
Matched 4553 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4516 matched stars entering correct_measured_positions(), 4517 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4516 matched stars entering correct_measured_positions(), 5888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 451 to 510 (Dec 0.4 to 11.7)
Done reading UCAC5 zone files...
Matched 4552 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4518 matched stars entering correct_measured_positions(), 5888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4518 matched stars entering correct_measured_positions(), 5888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4518 stars left (next iteration limit 4967)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4518 robust_rms=10.114 arcsec worst_quadrant_rms=14.335 arcsec
SIP_REFIT: SIP order 3 trial: matched=4518 robust_rms=0.386 arcsec worst_quadrant_rms=0.410 arcsec
SIP_REFIT: SIP order 5 trial: matched=4518 robust_rms=0.280 arcsec worst_quadrant_rms=0.310 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4518 robust_rms_before=0.869 arcsec robust_rms_before_corrected=0.329 arcsec robust_rms_after=0.280 arcsec worst_quadrant_rms_before=0.378 worst_quadrant_rms_after=0.310
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
Image size: 941.3'x626.8' 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: 22:17:04.654 +06:02:45.49 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5888 stars ###
'wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/correct_sextractor_wcs_catalog_usingxy2sky3705244.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.869 -> 0.280 arcsec)
WCS_QUALITY_DIAG: file=fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits N_match=4518 sigma_overall_arcsec=0.303 sigma_q1_arcsec=0.314 sigma_q2_arcsec=0.339 sigma_q3_arcsec=0.285 sigma_q4_arcsec=0.284 n_q1=1053 n_q2=1295 n_q3=928 n_q4=1242 worst_quadrant_to_overall_ratio=1.121
The image catalog is written to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits -region wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.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.0JmhcBBO2x (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_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.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_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
Checking if the catalog wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.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_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
WCS catalog name: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.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=353, bad_region=0, passed=5823
Got 5823 stars (including 5463 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits.wcscat
util/solve_plate_with_UCAC5 got 5823 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 4552 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4515 matched stars entering correct_measured_positions(), 4516 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4515 matched stars entering correct_measured_positions(), 5823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 4552 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4516 matched stars entering correct_measured_positions(), 5823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4516 matched stars entering correct_measured_positions(), 5823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4516 stars left (next iteration limit 4966)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4516 robust_rms=10.350 arcsec worst_quadrant_rms=14.169 arcsec
SIP_REFIT: SIP order 3 trial: matched=4516 robust_rms=0.399 arcsec worst_quadrant_rms=0.437 arcsec
SIP_REFIT: SIP order 5 trial: matched=4516 robust_rms=0.296 arcsec worst_quadrant_rms=0.326 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4516 robust_rms_before=0.876 arcsec robust_rms_before_corrected=0.341 arcsec robust_rms_after=0.296 arcsec worst_quadrant_rms_before=0.396 worst_quadrant_rms_after=0.326
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
Image size: 941.3'x626.8' 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: 22:17:02.128 +06:02:05.98 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5823 stars ###
'wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/correct_sextractor_wcs_catalog_usingxy2sky3705284.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.876 -> 0.296 arcsec)
WCS_QUALITY_DIAG: file=fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits N_match=4516 sigma_overall_arcsec=0.311 sigma_q1_arcsec=0.321 sigma_q2_arcsec=0.364 sigma_q3_arcsec=0.297 sigma_q4_arcsec=0.288 n_q1=1061 n_q2=1286 n_q3=932 n_q4=1237 worst_quadrant_to_overall_ratio=1.170
The image catalog is written to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits -region wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.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_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits to local_wcs_cache/
'wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits' -> 'local_wcs_cache/wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits'
Saving the final (post-refit) wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits to local_wcs_cache/
'wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits' -> 'local_wcs_cache/wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits'
Saving the final (post-refit) wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits to local_wcs_cache/
'wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits' -> 'local_wcs_cache/wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits'
Saving the final (post-refit) wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits to local_wcs_cache/
'wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits' -> 'local_wcs_cache/wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits sigma_overall=0.426 worst_q_ratio=1.083
ref2=Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits sigma_overall=0.464 worst_q_ratio=1.097
new1=fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits sigma_overall=0.303 worst_q_ratio=1.121
new2=fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits sigma_overall=0.311 worst_q_ratio=1.170
reference average sigma_overall=0.445 worst_q_ratio=1.09
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300_astrometric_residuals.png (4530 matched stars from wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493_astrometric_residuals.png (4515 matched stars from wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279_astrometric_residuals.png (4518 matched stars from wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280_astrometric_residuals.png (4516 matched stars from wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits'
Saving fully-calibrated image wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits'
Preparing the HTML report for the field Peg-11-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20923_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 20923_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
**** FOUND 22:31:14.67 +06:22:49.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04551_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 04551_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
**** FOUND 21:48:46.04 +07:12:18.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Peg-11-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
SExtractor catalog cache: saved Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.cat to cache
SExtractor catalog cache: saved Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Creating symlink local_wcs_cache/wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.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_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits exists and is non-empty
wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits exists and is non-empty
wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits exists and is non-empty
wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (1st reference image)
verification OK: wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:09.147 +06:00:12.37 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits (1st new image)
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
Image size: 941.3'x626.8' 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: 22:17:04.654 +06:02:45.49 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:17:09.147 +06:00:12.37
Second-epoch image center 22:17:04.654 +06:02:45.49
Angular distance between the image centers 0.0464 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits (2nd new image)
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
Image size: 941.3'x626.8' 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: 22:17:02.128 +06:02:05.98 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:17:09.147 +06:00:12.37
Second-epoch image center 22:17:02.128 +06:02:05.98
Angular distance between the image centers 0.0429 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 22:17:04.654 +06:02:45.49
Second-epoch second image center 22:17:02.128 +06:02:05.98
Angular distance between the image centers 0.01517 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/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits &> /tmp/tmp.TTaAuso8M4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits &> /tmp/tmp.3MeY8drX9j
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits &> /tmp/tmp.vHCgykyQdt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits &> /tmp/tmp.lujf1LgnbL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.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_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.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_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
Found non-empty wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
The reference image (wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits) and catalog (wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat) found
'wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat' -> 'wcsmag.cat'
Read 49086 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2980 to 342.2142 deg, Dec +0.6967 to +11.2720 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 326.2980 to 342.2142 deg, Dec 0.6967 to 11.2720 deg
Loaded 6047 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): 4866 out of 5316 total matches.
Matched with Tycho-2 5316 out of 49086 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.420900
a=0.000000 b=1.000000 c=22.420900
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.09
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 49086 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2980 to 342.2142 deg, Dec +0.6967 to +11.2720 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 326.2980 to 342.2142 deg, Dec 0.6967 to 11.2720 deg
Loaded 6047 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): 4866 out of 5316 total matches.
Matched with Tycho-2 5316 out of 49086 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Forced-photometry filter: calibrated wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits -> calib.txt_param_ref_wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (aperture=4.8)
Read 51877 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.3357 to 342.2473 deg, Dec +0.7146 to +11.2610 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 326.3357 to 342.2473 deg, Dec 0.7146 to 11.2610 deg
Loaded 6042 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): 4832 out of 5335 total matches.
Matched with Tycho-2 5335 out of 51877 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Forced-photometry filter: calibrated wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits -> calib.txt_param_ref_wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 50 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
2.1 pix Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
2.0 pix fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
2.0 pix fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
Limiting magnitude estimates:
15.1 mag. Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
15.2 mag. Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
14.8 mag. fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
14.8 mag. fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.TTaAuso8M4 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits' -> 'wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.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/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS-calibrated image found: wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Checking if the catalog wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS catalog name: wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.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=21, blended=2220, bad_region=0, passed=49065
Got 49065 stars (including 46775 good ones) from the SExtractor catalog wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 49065 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4544 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4519 matched stars entering correct_measured_positions(), 4519 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4519 matched stars entering correct_measured_positions(), 49065 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4544 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4518 matched stars entering correct_measured_positions(), 49065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4517 matched stars entering correct_measured_positions(), 49065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4517 stars left (next iteration limit 4970)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.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_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits N_match=4517 sigma_overall_arcsec=0.406 sigma_q1_arcsec=0.340 sigma_q2_arcsec=0.436 sigma_q3_arcsec=0.422 sigma_q4_arcsec=0.453 n_q1=1279 n_q2=891 n_q3=1277 n_q4=1070 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits -region wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.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.3MeY8drX9j (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits' -> 'wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.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/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS-calibrated image found: wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Checking if the catalog wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS catalog name: wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.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=30, blended=2471, bad_region=0, passed=51847
Got 51847 stars (including 49304 good ones) from the SExtractor catalog wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat
util/solve_plate_with_UCAC5 got 51847 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4538 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4511 matched stars entering correct_measured_positions(), 4511 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4511 matched stars entering correct_measured_positions(), 51847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4538 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4513 matched stars entering correct_measured_positions(), 51847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4513 matched stars entering correct_measured_positions(), 51847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4513 stars left (next iteration limit 4962)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.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_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits N_match=4513 sigma_overall_arcsec=0.438 sigma_q1_arcsec=0.368 sigma_q2_arcsec=0.482 sigma_q3_arcsec=0.406 sigma_q4_arcsec=0.483 n_q1=1055 n_q2=1343 n_q3=876 n_q4=1239 worst_quadrant_to_overall_ratio=1.103
The image catalog is written to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits -region wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.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.vHCgykyQdt (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_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.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_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
Checking if the catalog wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.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_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
WCS catalog name: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.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=18, blended=1413, bad_region=10, passed=41811
Got 41811 stars (including 40308 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits.wcscat
util/solve_plate_with_UCAC5 got 41811 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 4530 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4497 matched stars entering correct_measured_positions(), 4497 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4497 matched stars entering correct_measured_positions(), 41811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 4530 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4497 matched stars entering correct_measured_positions(), 41811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4497 matched stars entering correct_measured_positions(), 41811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4497 stars left (next iteration limit 4946)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.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=4497 robust_rms=10.076 arcsec worst_quadrant_rms=13.720 arcsec
SIP_REFIT: SIP order 3 trial: matched=4497 robust_rms=0.377 arcsec worst_quadrant_rms=0.399 arcsec
SIP_REFIT: SIP order 5 trial: matched=4497 robust_rms=0.274 arcsec worst_quadrant_rms=0.300 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4497 robust_rms_before=0.275 arcsec robust_rms_before_corrected=0.296 arcsec robust_rms_after=0.274 arcsec worst_quadrant_rms_before=0.300 worst_quadrant_rms_after=0.300
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.300 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits N_match=4497 sigma_overall_arcsec=0.305 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.355 sigma_q3_arcsec=0.258 sigma_q4_arcsec=0.284 n_q1=1077 n_q2=1285 n_q3=920 n_q4=1215 worst_quadrant_to_overall_ratio=1.164
The image catalog is written to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits -region wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.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.lujf1LgnbL (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_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.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_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
Checking if the catalog wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.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_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
WCS catalog name: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.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=9, blended=1442, bad_region=15, passed=42134
Got 42134 stars (including 40603 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits.wcscat
util/solve_plate_with_UCAC5 got 42134 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 4537 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4503 matched stars entering correct_measured_positions(), 4503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4503 matched stars entering correct_measured_positions(), 42134 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 4537 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4503 matched stars entering correct_measured_positions(), 42134 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4503 matched stars entering correct_measured_positions(), 42134 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4503 stars left (next iteration limit 4953)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.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=4503 robust_rms=10.086 arcsec worst_quadrant_rms=14.006 arcsec
SIP_REFIT: SIP order 3 trial: matched=4503 robust_rms=0.390 arcsec worst_quadrant_rms=0.419 arcsec
SIP_REFIT: SIP order 5 trial: matched=4503 robust_rms=0.287 arcsec worst_quadrant_rms=0.316 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4503 robust_rms_before=0.288 arcsec robust_rms_before_corrected=0.313 arcsec robust_rms_after=0.287 arcsec worst_quadrant_rms_before=0.318 worst_quadrant_rms_after=0.316
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.318 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits N_match=4503 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.354 sigma_q3_arcsec=0.281 sigma_q4_arcsec=0.300 n_q1=1078 n_q2=1291 n_q3=923 n_q4=1211 worst_quadrant_to_overall_ratio=1.128
The image catalog is written to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-03_CI_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits -region wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.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_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.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_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-24-45_20.00sec_0.00C_LIGHTs_0279.fits
Saving fully-calibrated image wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.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_Peg-11-Q1b1x1_063221_TTUQ1b1x1_3554997_uxYwuuhT/wcs_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280.fits
Preparing the HTML report for the field Peg-11-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:16:00.07 +10:48:21.7: 13.79 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:38:00.02 +07:52:38.1: 14.10 +/- 0.08 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:50:14.38 +06:12:00.2: 13.57 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:22:39.53 +05:00:35.2: 13.00 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:59:25.58 +10:06:10.7: 13.99 +/- 0.08 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:48:33.73 +10:55:19.7: 13.37 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:27:51.98 +03:56:37.4: 13.47 +/- 0.05 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:46:30.02 +07:09:23.5: 13.53 +/- 0.05 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:51:46.60 +09:41:47.5: 13.61 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:02:44.63 +08:29:44.7: 13.15 +/- 0.04 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:46:30.02 +07:09:23.5: 13.48 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:59:25.58 +10:06:10.7: 13.92 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:50:14.38 +06:12:00.2: 13.81 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:48:33.73 +10:55:19.7: 13.47 +/- 0.05 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:16:00.07 +10:48:21.7: 13.74 +/- 0.05 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:38:00.02 +07:52:38.1: 13.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:27:51.98 +03:56:37.4: 13.51 +/- 0.04 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:22:39.53 +05:00:35.2: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Forced photometry filter REJECTED candidate at 22:46:30.02 +07:09:23.5: ref_mag=13.51 +/- 0.04 new_mean_mag=13.7066 delta=-0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:59:25.58 +10:06:10.7: ref_mag=13.95 +/- 0.05 new_mean_mag=14.1494 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:51:46.60 +09:41:47.5: 13.49 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 21:50:14.38 +06:12:00.2: ref_mag=13.69 +/- 0.04 new_mean_mag=13.7046 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 13.42 +/- 0.04
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter REJECTED candidate at 21:48:33.73 +10:55:19.7: ref_mag=13.42 +/- 0.04 new_mean_mag=13.6183 delta=-0.19 (need > 0.90)
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry filter REJECTED candidate at 22:16:00.07 +10:48:21.7: ref_mag=13.76 +/- 0.04 new_mean_mag=14.1079 delta=-0.35 (need > 0.90)
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Forced photometry filter REJECTED candidate at 22:27:51.98 +03:56:37.4: ref_mag=13.49 +/- 0.03 new_mean_mag=13.7777 delta=-0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:22:39.53 +05:00:35.2: ref_mag=13.03 +/- 0.02 new_mean_mag=13.5472 delta=-0.52 (need > 0.90)
Forced photometry reference-image weighted average: 13.53 +/- 0.04
Forced photometry filter REJECTED candidate at 22:38:00.02 +07:52:38.1: ref_mag=13.95 +/- 0.05 new_mean_mag=13.9209 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:51:46.60 +09:41:47.5: ref_mag=13.53 +/- 0.04 new_mean_mag=13.7071 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:02:44.63 +08:29:44.7: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry filter REJECTED candidate at 22:02:44.63 +08:29:44.7: ref_mag=13.16 +/- 0.03 new_mean_mag=13.2107 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:24:56.80 +09:24:18.5: 12.88 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:45:37.93 +10:16:26.8: 12.79 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:16:02.34 +09:10:16.2: 12.69 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:59:47.62 +09:53:21.0: 12.72 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:06:25.39 +11:08:29.5: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:31:52.26 +03:51:04.0: 12.59 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:52:56.59 +09:57:48.1: 12.85 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:55:09.37 +10:08:56.5: 12.51 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:33:58.13 +09:10:57.8: 12.94 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:11:28.99 +09:43:18.6: 13.64 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:24:56.80 +09:24:18.5: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter REJECTED candidate at 22:24:56.80 +09:24:18.5: ref_mag=12.87 +/- 0.02 new_mean_mag=13.2719 delta=-0.40 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:31:52.26 +03:51:04.0: 12.28 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:59:47.62 +09:53:21.0: 12.97 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:45:37.93 +10:16:26.8: 12.68 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:16:02.34 +09:10:16.2: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Forced photometry filter REJECTED candidate at 21:59:47.62 +09:53:21.0: ref_mag=12.83 +/- 0.02 new_mean_mag=13.0187 delta=-0.19 (need > 0.90)
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Forced photometry filter REJECTED candidate at 22:31:52.26 +03:51:04.0: ref_mag=12.39 +/- 0.01 new_mean_mag=12.8664 delta=-0.47 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:52:56.59 +09:57:48.1: 12.84 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.02
Forced photometry filter REJECTED candidate at 22:45:37.93 +10:16:26.8: ref_mag=12.73 +/- 0.02 new_mean_mag=12.9845 delta=-0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:16:02.34 +09:10:16.2: ref_mag=12.69 +/- 0.02 new_mean_mag=12.9318 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:55:09.37 +10:08:56.5: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry filter REJECTED candidate at 21:52:56.59 +09:57:48.1: ref_mag=12.85 +/- 0.02 new_mean_mag=13.1535 delta=-0.31 (need > 0.90)
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:06:25.39 +11:08:29.5: 15.80 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 21:55:09.37 +10:08:56.5: ref_mag=12.54 +/- 0.01 new_mean_mag=12.8749 delta=-0.33 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:33:58.13 +09:10:57.8: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter REJECTED candidate at 22:33:58.13 +09:10:57.8: ref_mag=12.98 +/- 0.02 new_mean_mag=13.0200 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:11:28.99 +09:43:18.6: 13.56 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Forced photometry filter REJECTED candidate at 22:11:28.99 +09:43:18.6: ref_mag=13.59 +/- 0.04 new_mean_mag=13.5885 delta=0.00 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:46:26.22 +07:59:31.8: 13.35 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:30:48.22 +08:38:48.8: 13.48 +/- 0.05 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:53:10.24 +09:04:16.0: 13.41 +/- 0.05 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:56:46.57 +03:59:58.9: 13.41 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:24:44.30 +09:49:58.7: 13.71 +/- 0.07 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:50:34.11 +10:56:03.3: 13.46 +/- 0.07 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:38:21.21 +09:15:37.4: 13.94 +/- 0.09 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:46:26.22 +07:59:31.8: 13.52 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:21:57.94 +10:04:11.0: 13.97 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 21:46:26.22 +07:59:31.8: ref_mag=13.44 +/- 0.04 new_mean_mag=13.5252 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:30:48.22 +08:38:48.8: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Forced photometry filter REJECTED candidate at 22:30:48.22 +08:38:48.8: ref_mag=13.37 +/- 0.03 new_mean_mag=13.7239 delta=-0.36 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:53:10.24 +09:04:16.0: 13.58 +/- 0.05 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:56:46.57 +03:59:58.9: 13.66 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.04
Forced photometry filter REJECTED candidate at 21:53:10.24 +09:04:16.0: ref_mag=13.50 +/- 0.04 new_mean_mag=13.6753 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:24:44.30 +09:49:58.7: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.04
Forced photometry filter REJECTED candidate at 21:56:46.57 +03:59:58.9: ref_mag=13.53 +/- 0.04 new_mean_mag=13.6489 delta=-0.12 (need > 0.90)
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry filter REJECTED candidate at 22:24:44.30 +09:49:58.7: ref_mag=13.69 +/- 0.04 new_mean_mag=13.6646 delta=0.02 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:50:34.11 +10:56:03.3: 13.78 +/- 0.07 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:38:21.21 +09:15:37.4: 13.74 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.05
Forced photometry filter REJECTED candidate at 21:50:34.11 +10:56:03.3: ref_mag=13.61 +/- 0.05 new_mean_mag=13.6109 delta=-0.00 (need > 0.90)
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Forced photometry filter REJECTED candidate at 22:38:21.21 +09:15:37.4: ref_mag=13.82 +/- 0.05 new_mean_mag=14.0113 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:58:55.69 +07:39:57.8: 14.00 +/- 0.08 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:21:57.94 +10:04:11.0: 13.94 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.05
Forced photometry filter REJECTED candidate at 22:21:57.94 +10:04:11.0: ref_mag=13.96 +/- 0.05 new_mean_mag=14.1539 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:58:55.69 +07:39:57.8: 14.00 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.05
Forced photometry filter REJECTED candidate at 21:58:55.69 +07:39:57.8: ref_mag=14.00 +/- 0.05 new_mean_mag=14.0707 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:42:56.00 +01:10:17.0: 14.42 +/- 0.14 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:45:02.05 +06:39:42.1: 14.85 +/- 0.20 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:44:56.44 +08:27:09.3: 14.93 +/- 0.19 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:46:59.61 +07:20:54.3: 14.36 +/- 0.12 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:48:09.64 +10:18:34.0: 14.38 +/- 0.14 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:14:08.99 +09:03:44.9: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:47:18.62 +10:40:46.9: 14.46 +/- 0.15 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:42:56.00 +01:10:17.0: 14.08 +/- 0.11 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:42:41.21 +02:29:16.7: 15.11 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.09
Forced photometry filter REJECTED candidate at 22:42:56.00 +01:10:17.0: ref_mag=14.20 +/- 0.09 new_mean_mag=14.2638 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:45:02.05 +06:39:42.1: 14.52 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.12
Forced photometry filter REJECTED candidate at 22:45:02.05 +06:39:42.1: ref_mag=14.64 +/- 0.12 new_mean_mag=14.2746 delta=0.37 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:44:56.44 +08:27:09.3: 14.85 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.13
Forced photometry filter REJECTED candidate at 22:44:56.44 +08:27:09.3: ref_mag=14.89 +/- 0.13 new_mean_mag=14.4189 delta=0.47 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:46:59.61 +07:20:54.3: 14.21 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.08
Forced photometry filter REJECTED candidate at 22:46:59.61 +07:20:54.3: ref_mag=14.28 +/- 0.08 new_mean_mag=14.2845 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:48:09.64 +10:18:34.0: 14.59 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.10
Forced photometry filter REJECTED candidate at 21:48:09.64 +10:18:34.0: ref_mag=14.48 +/- 0.10 new_mean_mag=14.2524 delta=0.23 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:47:18.62 +10:40:46.9: 14.61 +/- 0.14 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:14:08.99 +09:03:44.9: 15.82 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.54 +/- 0.10
Forced photometry filter REJECTED candidate at 21:47:18.62 +10:40:46.9: ref_mag=14.54 +/- 0.10 new_mean_mag=14.3196 delta=0.22 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:40:45.55 +10:16:32.4: 15.04 +/- 0.22 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:42:41.21 +02:29:16.7: 15.00 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.16
Forced photometry filter REJECTED candidate at 22:42:41.21 +02:29:16.7: ref_mag=15.05 +/- 0.16 new_mean_mag=14.5821 delta=0.47 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:40:45.55 +10:16:32.4: 14.83 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.14
Forced photometry filter REJECTED candidate at 22:40:45.55 +10:16:32.4: ref_mag=14.91 +/- 0.14 new_mean_mag=14.5360 delta=0.37 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:46:52.25 +04:53:05.8: 14.49 +/- 0.14 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:29:18.68 +02:25:30.5: 14.88 +/- 0.18 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:24:07.28 +09:13:27.0: 15.10 +/- 0.20 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:52:35.83 +11:07:37.7: 99.00 +/- 99.00 edge
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:49:30.93 +11:04:38.3: 14.50 +/- 0.17 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:51:23.99 +09:52:22.2: 14.25 +/- 0.12 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:46:52.25 +04:53:05.8: 14.52 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.50 +/- 0.10
Forced photometry filter REJECTED candidate at 22:46:52.25 +04:53:05.8: ref_mag=14.50 +/- 0.10 new_mean_mag=14.5559 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:53:54.89 +08:24:17.9: 14.95 +/- 0.20 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:29:18.68 +02:25:30.5: 15.19 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.00 +/- 0.14
Forced photometry filter REJECTED candidate at 22:29:18.68 +02:25:30.5: ref_mag=15.00 +/- 0.14 new_mean_mag=14.6199 delta=0.38 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:24:07.28 +09:13:27.0: 14.91 +/- 0.16 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:52:35.83 +11:07:37.7: 14.71 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 21:52:35.83 +11:07:37.7: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry reference-image weighted average: 14.98 +/- 0.12
Forced photometry filter REJECTED candidate at 22:24:07.28 +09:13:27.0: ref_mag=14.98 +/- 0.12 new_mean_mag=14.6244 delta=0.36 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:49:30.93 +11:04:38.3: 14.39 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.09
Forced photometry filter REJECTED candidate at 21:49:30.93 +11:04:38.3: ref_mag=14.43 +/- 0.09 new_mean_mag=14.4184 delta=0.01 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:51:23.99 +09:52:22.2: 14.86 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.10
Forced photometry filter REJECTED candidate at 21:51:23.99 +09:52:22.2: ref_mag=14.44 +/- 0.10 new_mean_mag=14.4743 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:53:54.89 +08:24:17.9: 14.83 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.12
Forced photometry filter REJECTED candidate at 21:53:54.89 +08:24:17.9: ref_mag=14.88 +/- 0.12 new_mean_mag=14.4941 delta=0.38 (need > 0.90)
Adding exclusion_list_local.txt__out56609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57592.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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
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Considering the candidate 56196_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56196_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56197_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56197_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56199_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56199_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
Rejecting candidate due to large distance (26.4") between the two second-epoch detections
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Considering the candidate 56200_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56200_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56201_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56201_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56204_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56204_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56205_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56205_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56206_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56206_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56207_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56207_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56208_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56208_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56209_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56209_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56210_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56210_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56211_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56211_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56212_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56212_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56213_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56213_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56214_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56214_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56215_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56215_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56609_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
Preparing report for the candidate 56609_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
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Considering the candidate 56673_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56673_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
**** FOUND 22:35:35.04 +10:20:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56674_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56674_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 56722_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 56722_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57010_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57010_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57068_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57068_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57078_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57078_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57083_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57083_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57102_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57102_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57116_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57116_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57126_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57126_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57279_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57279_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57333_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57333_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
**** FOUND 21:48:32.73 +07:09:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57399_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57399_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57417_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57417_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57472_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57472_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57490_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57490_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57517_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57517_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57549_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57549_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57552_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57552_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57592_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
Preparing report for the candidate 57592_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
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Considering the candidate 57660_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57660_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57678_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57678_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57685_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57685_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57686_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57686_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57725_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57725_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57743_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57743_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57745_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57745_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57773_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57773_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57775_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57775_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 57809_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 57809_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
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Considering the candidate 36115_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 36115_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks
**** FOUND 21:48:46.19 +07:12:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24406_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280
The candidate 24406_fd_Peg-11-Q1b1x1_2026-09-03_02-25-51_20.00sec_-0.00C_LIGHTs_0280 did not pass the final checks