This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0
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 10 12.2135 2461325.7135 11.91 22:22:20.41 +07:25:30.4
71.26288 -40.04111 galactic Peg Second-epoch detections are separated by 0.4" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.690 Wratislavia 0 1 1 12.3 0 0
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:22:20.41 +07:25:30.4: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:22:20.41 +07:25:30.4: 15.71 +/- 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,2461325.7135,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261012.2135 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.2135 2461325.7135 14.59 22:27:12.60 +09:14:38.2
74.03301 -39.56124 galactic Peg Second-epoch detections are separated by 2.4" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1243 Pamela -0 0 0 14.5 -0 -0
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:27:12.60 +09:14:38.2: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:27:12.60 +09:14:38.2: 15.83 +/- 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,2461325.7135,14.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261012.2135 14.59CV 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-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Last image: 2461325.71376194 12.10.2026 05:07:39.032 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 12 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): 6675
Objects passed selection criteria: 6670
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: 6470.75
Average stars matched: 5667.5 (87.5864 %)
Memory usage VmPeak: 234392 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Oct 12 00:47:23 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-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Last image: 2461325.71376194 12.10.2026 05:07:39.032 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 120
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.06
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: 61 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): 43281
Objects passed selection criteria: 43180
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: 42496.5
Average stars matched: 37641.5 (88.5755 %)
Memory usage VmPeak: 268600 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Oct 12 00:50:15 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
SExtractor catalog cache: saved Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.cat to cache
SExtractor catalog cache: saved Peg-11-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461325.71330083
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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits exists and is non-empty
wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits exists and is non-empty
wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits exists and is non-empty
wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (1st reference image)
verification OK: wcs_Peg-11-Q2b1x1_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-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits (1st new image)
verification OK: wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
Image size: 937.0'x624.0' 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: 22:17:09.022 +05:59:59.48 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 22:17:09.022 +05:59:59.48
Angular distance between the image centers 0.0036 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits (2nd new image)
verification OK: wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
Image size: 937.0'x624.0' 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: 22:17:10.189 +05:59:49.38 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 22:17:10.189 +05:59:49.38
Angular distance between the image centers 0.0077 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 22:17:09.022 +05:59:59.48
Second-epoch second image center 22:17:10.189 +05:59:49.38
Angular distance between the image centers 0.00559 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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits &> /tmp/tmp.1sjCKjc2pg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits &> /tmp/tmp.vOICp3pUWw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_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_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits &> /tmp/tmp.LuGtmGlzeX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits &> /tmp/tmp.2hzAtkPoxk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-11-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
Found non-empty wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
The reference image (wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits) and catalog (wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat) found
'wcs_Peg-11-Q2b1x1_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 22.552300
a=0.000000 b=1.000000 c=22.552300
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.19
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.19
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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Forced-photometry filter: calibrated wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits -> calib.txt_param_ref_wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (aperture=6.2)
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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Forced-photometry filter: calibrated wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits -> calib.txt_param_ref_wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
2.3 pix Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
2.3 pix fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
2.3 pix fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
Limiting magnitude estimates:
15.2 mag. Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
15.3 mag. Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
15.5 mag. fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
15.5 mag. fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 12.0 (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.1sjCKjc2pg (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits' -> 'wcs_Peg-11-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS-calibrated image found: wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Checking if the catalog wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS catalog name: wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=416, bad_region=1477, passed=7642
Got 7642 stars (including 5810 good ones) from the SExtractor catalog wcs_Peg-11-Q2b1x1_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 4598 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4570 matched stars entering correct_measured_positions(), 4570 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4570 matched stars entering correct_measured_positions(), 6432 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4598 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4569 matched stars entering correct_measured_positions(), 6432 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4569 matched stars entering correct_measured_positions(), 6432 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4569 stars left (next iteration limit 5027)
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-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits N_match=4569 sigma_overall_arcsec=0.393 sigma_q1_arcsec=0.341 sigma_q2_arcsec=0.385 sigma_q3_arcsec=0.443 sigma_q4_arcsec=0.400 n_q1=1546 n_q2=653 n_q3=1614 n_q4=756 worst_quadrant_to_overall_ratio=1.128
The image catalog is written to wcs_Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits -region wcs_Peg-11-Q2b1x1_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-Q2b1x1_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.vOICp3pUWw (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits' -> 'wcs_Peg-11-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS-calibrated image found: wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Checking if the catalog wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat corresponding to the image wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat corresponding to the image wcs_Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS catalog name: wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=449, bad_region=2308, passed=8182
Got 8182 stars (including 5505 good ones) from the SExtractor catalog wcs_Peg-11-Q2b1x1_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 4523 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4490 matched stars entering correct_measured_positions(), 4490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4490 matched stars entering correct_measured_positions(), 6364 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 4523 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4490 matched stars entering correct_measured_positions(), 6364 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4490 matched stars entering correct_measured_positions(), 6364 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4490 stars left (next iteration limit 4939)
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-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits N_match=4490 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.376 sigma_q2_arcsec=0.428 sigma_q3_arcsec=0.418 sigma_q4_arcsec=0.390 n_q1=1433 n_q2=1007 n_q3=1183 n_q4=867 worst_quadrant_to_overall_ratio=1.055
The image catalog is written to wcs_Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits -region wcs_Peg-11-Q2b1x1_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-Q2b1x1_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.LuGtmGlzeX (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_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.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_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
Checking if the catalog wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
WCS catalog name: wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=529, bad_region=2677, passed=9648
Got 9648 stars (including 6529 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat
util/solve_plate_with_UCAC5 got 9648 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 4520 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4488 matched stars entering correct_measured_positions(), 4488 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4488 matched stars entering correct_measured_positions(), 7548 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 4520 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4487 matched stars entering correct_measured_positions(), 7548 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4487 matched stars entering correct_measured_positions(), 7548 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4487 stars left (next iteration limit 4936)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4487 robust_rms=7.959 arcsec worst_region_rms=20.609 arcsec outer_annulus_rms=20.609 arcsec
SIP_REFIT: SIP order 3 trial: matched=4487 robust_rms=0.438 arcsec worst_region_rms=0.993 arcsec outer_annulus_rms=0.993 arcsec
SIP_REFIT: SIP order 5 trial: matched=4487 robust_rms=0.349 arcsec worst_region_rms=0.415 arcsec outer_annulus_rms=0.415 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4487 robust_rms_before=0.873 arcsec robust_rms_before_corrected=0.368 arcsec robust_rms_after=0.349 arcsec worst_region_rms_before=0.446 worst_region_rms_after=0.415 outer_annulus_rms_before=1.135 outer_annulus_rms_after=0.415
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.446 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits worst_region_rms_kept=0.446 arcsec robust_rms_kept=0.368 arcsec matched=4487
WCS_QUALITY_DIAG: file=fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits N_match=4487 sigma_overall_arcsec=0.383 sigma_q1_arcsec=0.348 sigma_q2_arcsec=0.436 sigma_q3_arcsec=0.387 sigma_q4_arcsec=0.381 n_q1=1446 n_q2=1009 n_q3=1165 n_q4=867 worst_quadrant_to_overall_ratio=1.136
The image catalog is written to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits -region wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.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.2hzAtkPoxk (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_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.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_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
Checking if the catalog wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
WCS catalog name: wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=543, bad_region=2659, passed=9682
Got 9682 stars (including 6585 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat
util/solve_plate_with_UCAC5 got 9682 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 4513 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4482 matched stars entering correct_measured_positions(), 4482 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4482 matched stars entering correct_measured_positions(), 7594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 4514 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4482 matched stars entering correct_measured_positions(), 7594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4482 matched stars entering correct_measured_positions(), 7594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4482 stars left (next iteration limit 4930)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4482 robust_rms=8.035 arcsec worst_region_rms=20.631 arcsec outer_annulus_rms=20.631 arcsec
SIP_REFIT: SIP order 3 trial: matched=4482 robust_rms=0.422 arcsec worst_region_rms=0.918 arcsec outer_annulus_rms=0.918 arcsec
SIP_REFIT: SIP order 5 trial: matched=4482 robust_rms=0.327 arcsec worst_region_rms=0.392 arcsec outer_annulus_rms=0.392 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4482 robust_rms_before=0.858 arcsec robust_rms_before_corrected=0.344 arcsec robust_rms_after=0.327 arcsec worst_region_rms_before=0.405 worst_region_rms_after=0.392 outer_annulus_rms_before=1.121 outer_annulus_rms_after=0.392
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.405 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits worst_region_rms_kept=0.405 arcsec robust_rms_kept=0.344 arcsec matched=4482
WCS_QUALITY_DIAG: file=fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits N_match=4482 sigma_overall_arcsec=0.358 sigma_q1_arcsec=0.324 sigma_q2_arcsec=0.394 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.371 n_q1=1443 n_q2=1007 n_q3=1168 n_q4=864 worst_quadrant_to_overall_ratio=1.102
The image catalog is written to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits -region wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits to local_wcs_cache/
'wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits' -> 'local_wcs_cache/wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits'
Saving the final (post-refit) wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits to local_wcs_cache/
'wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits' -> 'local_wcs_cache/wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits'
Saving the final (post-refit) wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits to local_wcs_cache/
'wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits' -> 'local_wcs_cache/wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits'
Saving the final (post-refit) wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits to local_wcs_cache/
'wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits' -> 'local_wcs_cache/wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits sigma_overall=0.393 worst_q_ratio=1.128
ref2=Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits sigma_overall=0.405 worst_q_ratio=1.055
new1=fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits sigma_overall=0.383 worst_q_ratio=1.136
new2=fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits sigma_overall=0.358 worst_q_ratio=1.102
reference average sigma_overall=0.399 worst_q_ratio=1.0915
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300_astrometric_residuals.png (4569 matched stars from wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493_astrometric_residuals.png (4490 matched stars from wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270_astrometric_residuals.png (4487 matched stars from wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271_astrometric_residuals.png (4482 matched stars from wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits'
Saving fully-calibrated image wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits'
Preparing the HTML report for the field Peg-11-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:12:28.92 +08:03:34.9: 12.55 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:12:33.26 +06:01:59.6: 11.95 +/- 0.01 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:13:24.87 +04:45:51.8: 11.19 +/- 0.01 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:22:20.41 +07:25:30.4: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:14:14.65 +08:55:44.3: 12.05 +/- 0.01 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:14:14.65 +08:55:44.3: 12.06 +/- 0.01 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:13:24.87 +04:45:51.8: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:12:33.26 +06:01:59.6: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.00
Forced photometry filter REJECTED candidate at 22:14:14.65 +08:55:44.3: ref_mag=12.05 +/- 0.01 new_mean_mag=12.0707 delta=-0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:13:24.87 +04:45:51.8: ref_mag=11.22 +/- 0.00 new_mean_mag=11.5868 delta=-0.37 (need > 0.90)
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Forced photometry filter REJECTED candidate at 22:12:33.26 +06:01:59.6: ref_mag=11.94 +/- 0.01 new_mean_mag=12.0329 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:22:20.41 +07:25:30.4: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:12:28.92 +08:03:34.9: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Forced photometry filter REJECTED candidate at 22:12:28.92 +08:03:34.9: ref_mag=12.73 +/- 0.02 new_mean_mag=11.9454 delta=0.78 (need > 0.90)
Adding exclusion_list_local.txt__out21857.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 13s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21853_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 21853_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21856_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 21856_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21857_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
Preparing report for the candidate 21857_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21858_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 21858_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21860_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 21860_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 16s
Prepared the HTML report for the field Peg-11-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
22:22:20.41 +07:25:30.4
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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
SExtractor catalog cache: saved Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.cat to cache
SExtractor catalog cache: saved Peg-11-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Creating symlink local_wcs_cache/wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
Checking 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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits exists and is non-empty
wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits exists and is non-empty
wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits exists and is non-empty
wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (1st reference image)
verification OK: wcs_Peg-11-Q2b1x1_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-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits (1st new image)
verification OK: wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
Image size: 937.0'x624.0' 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: 22:17:09.022 +05:59:59.48 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 22:17:09.022 +05:59:59.48
Angular distance between the image centers 0.0036 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits (2nd new image)
verification OK: wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
Image size: 937.0'x624.0' 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: 22:17:10.189 +05:59:49.38 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 22:17:10.189 +05:59:49.38
Angular distance between the image centers 0.0077 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 22:17:09.022 +05:59:59.48
Second-epoch second image center 22:17:10.189 +05:59:49.38
Angular distance between the image centers 0.00559 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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits &> /tmp/tmp.TqPipWIilj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits &> /tmp/tmp.UQ4FSZ3SZ5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_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_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits &> /tmp/tmp.et4LmCWsGt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits &> /tmp/tmp.Vsywj1ViuV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-11-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
Found non-empty wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
The reference image (wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits) and catalog (wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat) found
'wcs_Peg-11-Q2b1x1_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 22.409850
a=0.000000 b=1.000000 c=22.409850
From vast_summary.log: estimated ref. image limiting mag.: -7.06
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.35
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.35
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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Forced-photometry filter: calibrated wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits -> calib.txt_param_ref_wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (aperture=4.7)
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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Forced-photometry filter: calibrated wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits -> calib.txt_param_ref_wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 81 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
2.1 pix Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
2.1 pix fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
2.1 pix fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
Limiting magnitude estimates:
15.4 mag. Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
15.5 mag. Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
15.6 mag. fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
15.6 mag. fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
All-image limiting magnitude estimate: 15.6 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.TqPipWIilj (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits' -> 'wcs_Peg-11-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS-calibrated image found: wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Checking if the catalog wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS catalog name: wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2220, bad_region=7484, passed=49070
Got 49070 stars (including 39704 good ones) from the SExtractor catalog wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 49070 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 4579 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4557 matched stars entering correct_measured_positions(), 4557 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4557 matched stars entering correct_measured_positions(), 43312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4579 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4555 matched stars entering correct_measured_positions(), 43312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4555 matched stars entering correct_measured_positions(), 43312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4555 stars left (next iteration limit 5012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits N_match=4555 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.339 sigma_q2_arcsec=0.369 sigma_q3_arcsec=0.426 sigma_q4_arcsec=0.388 n_q1=1549 n_q2=649 n_q3=1567 n_q4=790 worst_quadrant_to_overall_ratio=1.123
The image catalog is written to wcs_Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits -region wcs_Peg-11-Q2b1x1_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-Q2b1x1_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.UQ4FSZ3SZ5 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits' -> 'wcs_Peg-11-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS-calibrated image found: wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Checking if the catalog wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat corresponding to the image wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat corresponding to the image wcs_Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS catalog name: wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2472, bad_region=11412, passed=51861
Got 51861 stars (including 38546 good ones) from the SExtractor catalog wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat
util/solve_plate_with_UCAC5 got 51861 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 4508 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4482 matched stars entering correct_measured_positions(), 4482 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4482 matched stars entering correct_measured_positions(), 43280 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 4508 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4482 matched stars entering correct_measured_positions(), 43280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4482 matched stars entering correct_measured_positions(), 43280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4482 stars left (next iteration limit 4930)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits N_match=4482 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.366 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.406 sigma_q4_arcsec=0.374 n_q1=1423 n_q2=1019 n_q3=1162 n_q4=878 worst_quadrant_to_overall_ratio=1.047
The image catalog is written to wcs_Peg-11-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits -region wcs_Peg-11-Q2b1x1_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-Q2b1x1_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.et4LmCWsGt (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_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.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_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
Checking if the catalog wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
WCS catalog name: wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=3088, bad_region=11030, passed=55754
Got 55754 stars (including 42630 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat
util/solve_plate_with_UCAC5 got 55754 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 4510 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4485 matched stars entering correct_measured_positions(), 4485 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4485 matched stars entering correct_measured_positions(), 47477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4508 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4485 matched stars entering correct_measured_positions(), 47477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4485 matched stars entering correct_measured_positions(), 47477 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4485 stars left (next iteration limit 4933)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.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=4485 robust_rms=7.943 arcsec worst_region_rms=20.037 arcsec outer_annulus_rms=20.037 arcsec
SIP_REFIT: SIP order 3 trial: matched=4485 robust_rms=0.438 arcsec worst_region_rms=0.996 arcsec outer_annulus_rms=0.996 arcsec
SIP_REFIT: SIP order 5 trial: matched=4485 robust_rms=0.344 arcsec worst_region_rms=0.418 arcsec outer_annulus_rms=0.418 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4485 robust_rms_before=0.873 arcsec robust_rms_before_corrected=0.363 arcsec robust_rms_after=0.344 arcsec worst_region_rms_before=0.459 worst_region_rms_after=0.418 outer_annulus_rms_before=1.148 outer_annulus_rms_after=0.418
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.459 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits worst_region_rms_kept=0.459 arcsec robust_rms_kept=0.363 arcsec matched=4485
WCS_QUALITY_DIAG: file=fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits N_match=4485 sigma_overall_arcsec=0.380 sigma_q1_arcsec=0.342 sigma_q2_arcsec=0.418 sigma_q3_arcsec=0.387 sigma_q4_arcsec=0.385 n_q1=1461 n_q2=996 n_q3=1170 n_q4=858 worst_quadrant_to_overall_ratio=1.098
The image catalog is written to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits -region wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.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.Vsywj1ViuV (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_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.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_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
Checking if the catalog wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
WCS catalog name: wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=3047, bad_region=10918, passed=55174
Got 55174 stars (including 42171 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat
util/solve_plate_with_UCAC5 got 55174 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 4512 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4485 matched stars entering correct_measured_positions(), 4485 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4485 matched stars entering correct_measured_positions(), 47012 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 4512 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4486 matched stars entering correct_measured_positions(), 47012 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4486 matched stars entering correct_measured_positions(), 47012 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4486 stars left (next iteration limit 4933)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.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=4486 robust_rms=7.966 arcsec worst_region_rms=20.073 arcsec outer_annulus_rms=20.073 arcsec
SIP_REFIT: SIP order 3 trial: matched=4486 robust_rms=0.417 arcsec worst_region_rms=0.929 arcsec outer_annulus_rms=0.929 arcsec
SIP_REFIT: SIP order 5 trial: matched=4486 robust_rms=0.323 arcsec worst_region_rms=0.393 arcsec outer_annulus_rms=0.393 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4486 robust_rms_before=0.859 arcsec robust_rms_before_corrected=0.338 arcsec robust_rms_after=0.323 arcsec worst_region_rms_before=0.424 worst_region_rms_after=0.393 outer_annulus_rms_before=1.118 outer_annulus_rms_after=0.393
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.424 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits worst_region_rms_kept=0.424 arcsec robust_rms_kept=0.338 arcsec matched=4486
WCS_QUALITY_DIAG: file=fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits N_match=4486 sigma_overall_arcsec=0.355 sigma_q1_arcsec=0.321 sigma_q2_arcsec=0.399 sigma_q3_arcsec=0.344 sigma_q4_arcsec=0.362 n_q1=1455 n_q2=987 n_q3=1174 n_q4=870 worst_quadrant_to_overall_ratio=1.122
The image catalog is written to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits -region wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.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-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.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_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-06-59_20.00sec_-0.00C_LIGHT_0270.fits
Saving fully-calibrated image wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.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_2026-10-12_CI_Peg-11-Q2b1x1_004443_TTUQ2b1x1_3884652_Z9VhhCW0/wcs_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271.fits
Preparing the HTML report for the field Peg-11-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:34:41.05 +07:16:11.7: 14.09 +/- 0.08 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:27:52.00 +03:56:39.5: 13.60 +/- 0.05 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:06:23.17 +08:47:03.7: 14.41 +/- 0.11 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:00:30.14 +04:13:13.9: 14.36 +/- 0.11 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:09:51.11 +05:52:39.6: 13.16 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:24:56.76 +09:24:19.0: 12.87 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:28:15.61 +03:45:42.6: 14.49 +/- 0.11 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:09:51.11 +05:52:39.6: 13.27 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:27:52.00 +03:56:39.5: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:24:56.76 +09:24:19.0: 12.89 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:34:41.05 +07:16:11.7: 14.26 +/- 0.09 detection
Forced photometry filter REJECTED candidate at 22:09:51.11 +05:52:39.6: ref_mag=13.21 +/- 0.02 new_mean_mag=13.6942 delta=-0.48 (need > 0.90)
Forced photometry reference-image weighted average: 13.62 +/- 0.04
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:06:23.17 +08:47:03.7: 14.60 +/- 0.11 detection
Forced photometry filter REJECTED candidate at 22:27:52.00 +03:56:39.5: ref_mag=13.62 +/- 0.04 new_mean_mag=13.8767 delta=-0.25 (need > 0.90)
Forced photometry reference-image weighted average: 14.17 +/- 0.06
Forced photometry filter REJECTED candidate at 22:24:56.76 +09:24:19.0: ref_mag=12.88 +/- 0.02 new_mean_mag=13.1599 delta=-0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:34:41.05 +07:16:11.7: ref_mag=14.17 +/- 0.06 new_mean_mag=14.3572 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:00:30.14 +04:13:13.9: 14.28 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.07
Forced photometry reference-image weighted average: 14.51 +/- 0.08
Forced photometry filter REJECTED candidate at 22:00:30.14 +04:13:13.9: ref_mag=14.31 +/- 0.07 new_mean_mag=14.4326 delta=-0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:06:23.17 +08:47:03.7: ref_mag=14.51 +/- 0.08 new_mean_mag=14.7416 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:28:15.61 +03:45:42.6: 14.45 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.08
Forced photometry filter REJECTED candidate at 22:28:15.61 +03:45:42.6: ref_mag=14.46 +/- 0.08 new_mean_mag=14.6459 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:31:35.59 +09:13:03.8: 13.42 +/- 0.05 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:31:35.59 +09:13:03.8: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Forced photometry filter REJECTED candidate at 22:31:35.59 +09:13:03.8: ref_mag=13.41 +/- 0.03 new_mean_mag=13.4076 delta=0.01 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:34:23.75 +03:44:30.9: 14.70 +/- 0.15 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:03:39.83 +04:23:49.7: 14.21 +/- 0.10 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:34:23.75 +03:44:30.9: 14.58 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.11
Forced photometry filter REJECTED candidate at 22:34:23.75 +03:44:30.9: ref_mag=14.64 +/- 0.11 new_mean_mag=14.3891 delta=0.25 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:03:39.83 +04:23:49.7: 14.43 +/- 0.11 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:33:40.50 +08:40:11.3: 14.95 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.08
Forced photometry filter REJECTED candidate at 22:03:39.83 +04:23:49.7: ref_mag=14.31 +/- 0.08 new_mean_mag=14.2885 delta=0.02 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:30:16.25 +07:52:59.3: 14.75 +/- 0.15 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:33:40.50 +08:40:11.3: 15.01 +/- 0.18 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:04:07.10 +01:58:33.9: 14.37 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.13
Forced photometry filter REJECTED candidate at 22:33:40.50 +08:40:11.3: ref_mag=14.98 +/- 0.13 new_mean_mag=14.6308 delta=0.35 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:33:47.63 +02:12:12.2: 14.91 +/- 0.18 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:28:51.61 +01:53:54.3: 14.66 +/- 0.14 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:30:16.25 +07:52:59.3: 15.03 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.12
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:34:24.63 +02:56:36.2: 14.90 +/- 0.17 detection
Forced photometry filter REJECTED candidate at 22:30:16.25 +07:52:59.3: ref_mag=14.86 +/- 0.12 new_mean_mag=14.5123 delta=0.35 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:04:07.10 +01:58:33.9: 14.40 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.39 +/- 0.09
Forced photometry filter REJECTED candidate at 22:04:07.10 +01:58:33.9: ref_mag=14.39 +/- 0.09 new_mean_mag=14.4183 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:34:48.61 +01:57:34.4: 14.97 +/- 0.20 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:27:12.60 +09:14:38.2: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:33:47.63 +02:12:12.2: 14.64 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.11
Forced photometry filter REJECTED candidate at 22:33:47.63 +02:12:12.2: ref_mag=14.75 +/- 0.11 new_mean_mag=14.6232 delta=0.13 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:04:43.81 +02:36:58.7: 15.06 +/- 0.21 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:28:51.61 +01:53:54.3: 14.61 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.64 +/- 0.10
Forced photometry filter REJECTED candidate at 22:28:51.61 +01:53:54.3: ref_mag=14.64 +/- 0.10 new_mean_mag=14.4179 delta=0.22 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:34:24.63 +02:56:36.2: 14.96 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.13
Forced photometry filter REJECTED candidate at 22:34:24.63 +02:56:36.2: ref_mag=14.93 +/- 0.13 new_mean_mag=14.6945 delta=0.24 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:27:12.60 +09:14:38.2: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:34:48.61 +01:57:34.4: 15.08 +/- 0.22 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:04:43.81 +02:36:58.7: 14.71 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.82 +/- 0.11
Forced photometry filter REJECTED candidate at 22:04:43.81 +02:36:58.7: ref_mag=14.82 +/- 0.11 new_mean_mag=14.6131 delta=0.20 (need > 0.90)
Forced photometry reference-image weighted average: 15.02 +/- 0.15
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:27:45.11 +04:38:23.6: 14.66 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 22:34:48.61 +01:57:34.4: ref_mag=15.02 +/- 0.15 new_mean_mag=14.7340 delta=0.29 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:05:01.04 +09:27:51.6: 14.59 +/- 0.14 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:09:20.94 +02:34:22.5: 14.82 +/- 0.17 detection
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:27:45.11 +04:38:23.6: 14.54 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.10
Forced photometry filter REJECTED candidate at 22:27:45.11 +04:38:23.6: ref_mag=14.59 +/- 0.10 new_mean_mag=14.7027 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:05:01.04 +09:27:51.6: 14.65 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.09
Forced photometry filter REJECTED candidate at 22:05:01.04 +09:27:51.6: ref_mag=14.63 +/- 0.09 new_mean_mag=14.5776 delta=0.05 (need > 0.90)
Forced photometry on wcs_Peg-11-Q2b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:09:20.94 +02:34:22.5: 14.99 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.12
Forced photometry filter REJECTED candidate at 22:09:20.94 +02:34:22.5: ref_mag=14.90 +/- 0.12 new_mean_mag=14.6626 delta=0.24 (need > 0.90)
Adding exclusion_list_local.txt__out62729.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62324_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62324_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62328_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62328_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62332_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62332_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62336_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62336_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62355_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62355_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62364_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62364_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62367_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62367_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62374_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62374_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
**** FOUND 22:02:44.63 +08:29:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62376_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62376_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62383_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62383_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62384_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62384_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62392_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62392_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
**** FOUND 22:22:20.41 +07:25:30.0 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62395_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62395_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62405_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62405_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62406_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62406_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
**** FOUND 22:19:34.61 +09:06:37.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62408_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62408_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62413_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62413_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62415_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62415_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62418_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62418_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62424_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62424_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62428_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62428_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62435_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62435_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62443_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62443_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62444_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62444_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62446_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62446_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62448_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62448_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62451_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62451_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62452_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62452_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62453_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62453_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62455_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62455_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62459_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62459_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62460_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62460_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62462_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62462_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62464_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62464_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62465_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62465_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62466_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62466_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62473_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62473_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62474_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62474_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62482_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62482_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62487_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62487_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62488_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62488_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62492_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62492_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62495_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62495_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62496_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62496_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62499_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62499_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62501_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62501_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62506_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62506_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62516_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62516_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62523_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62523_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62530_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62530_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62539_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62539_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62549_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62549_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62566_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62566_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62570_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62570_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62571_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62571_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62573_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62573_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62575_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62575_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62576_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62576_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62583_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62583_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62598_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62598_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62602_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62602_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62612_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62612_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62614_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62614_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62624_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62624_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62628_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62628_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62630_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62630_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62639_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62639_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62655_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62655_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62656_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62656_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62674_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62674_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62690_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62690_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62712_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62712_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62721_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62721_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62729_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
Preparing report for the candidate 62729_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62734_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62734_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62745_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62745_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62803_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62803_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62849_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62849_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62856_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 62856_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24406_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 24406_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks
**** FOUND 22:31:14.58 +06:22:49.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58927_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271
The candidate 58927_fd_Peg-11-Q2b1x1_2026-10-12_00-07-39_20.00sec_0.00C_LIGHT_0271 did not pass the final checks