This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 06.3696 2461289.8696 12.49 22:04:46.10 +10:31:51.3
70.21161 -34.77110 galactic Peg Second-epoch detections are separated by 0.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.225 Henrietta 0 0 0 12.5 -0 0
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:04:46.10 +10:31:51.3: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:04:46.10 +10:31:51.3: 15.74 +/- 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,2461289.8696,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260906.3696 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.3696 2461289.8696 14.20 22:11:10.01 +09:27:31.0
70.61666 -36.64815 galactic Peg Second-epoch detections are separated by 1.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.105158 2000 OL -0 -0 0 14.3 0 0
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:11:10.01 +09:27:31.0: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:11:10.01 +09:27:31.0: 15.79 +/- 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,2461289.8696,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260906.3696 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461239.82973319 18.07.2026 07:54:38.948 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
First image: 2461239.82973319 18.07.2026 07:54:38.948 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Last image: 2461289.86992212 06.09.2026 08:52:31.271 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 7977
Objects passed selection criteria: 7973
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 7327.25
Average stars matched: 7005.5 (95.6089 %)
Memory usage VmPeak: 233736 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 6 03:54:20 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461239.82973319 18.07.2026 07:54:38.948 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
First image: 2461239.82973319 18.07.2026 07:54:38.948 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Last image: 2461289.86992212 06.09.2026 08:52:31.271 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 63
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 16 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): 50136
Objects passed selection criteria: 49987
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: 46003.2
Average stars matched: 43594.5 (94.764 %)
Memory usage VmPeak: 269700 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 6 03:55:10 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
SExtractor catalog cache: saved Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.cat to cache
SExtractor catalog cache: saved Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461289.86923965
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits exists and is non-empty
wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits exists and is non-empty
wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits exists and is non-empty
wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (1st reference image)
verification OK: wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:09.147 +06:00:12.37 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits (1st new image)
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:18.937 +05:58:15.98 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 22:17:18.937 +05:58:15.98
Angular distance between the image centers 0.0519 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits (2nd new image)
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:16.725 +05:58:31.91 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 22:17:16.725 +05:58:31.91
Angular distance between the image centers 0.0420 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 22:17:18.937 +05:58:15.98
Second-epoch second image center 22:17:16.725 +05:58:31.91
Angular distance between the image centers 0.01018 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits &> /tmp/tmp.1vS30AiNqP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits &> /tmp/tmp.MEdLzjhIxe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits &> /tmp/tmp.auvuw6XVCt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits &> /tmp/tmp.MaNIxqbXEf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
Found non-empty wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
The reference image (wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits) and catalog (wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat) found
'wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat' -> 'wcsmag.cat'
Read 7642 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.3157 to 342.2143 deg, Dec +0.7081 to +11.2594 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.3157 to 342.2143 deg, Dec 0.7081 to 11.2594 deg
Loaded 6032 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4873 out of 5003 total matches.
Matched with Tycho-2 5003 out of 7642 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.558200
a=0.000000 b=1.000000 c=22.558200
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.94
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.94
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7642 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.3157 to 342.2143 deg, Dec +0.7081 to +11.2594 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.3157 to 342.2143 deg, Dec 0.7081 to 11.2594 deg
Loaded 6032 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4873 out of 5003 total matches.
Matched with Tycho-2 5003 out of 7642 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Forced-photometry filter: calibrated wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits -> calib.txt_param_ref_wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (aperture=6.3)
Read 8182 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.3433 to 342.2304 deg, Dec +0.7273 to +11.2580 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.3433 to 342.2304 deg, Dec 0.7273 to 11.2580 deg
Loaded 6015 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4922 out of 5084 total matches.
Matched with Tycho-2 5084 out of 8182 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Forced-photometry filter: calibrated wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits -> calib.txt_param_ref_wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
2.3 pix Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
2.5 pix fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
2.5 pix fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
Limiting magnitude estimates:
14.9 mag. Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
15.0 mag. Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
14.9 mag. fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
14.9 mag. fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 11.9 (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.1vS30AiNqP (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits' -> 'wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS-calibrated image found: wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Checking if the catalog wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS catalog name: wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=416, bad_region=0, passed=7642
Got 7642 stars (including 7221 good ones) from the SExtractor catalog wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 7642 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4564 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4531 matched stars entering correct_measured_positions(), 4531 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4531 matched stars entering correct_measured_positions(), 7642 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4564 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4530 matched stars entering correct_measured_positions(), 7642 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4530 matched stars entering correct_measured_positions(), 7642 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4530 stars left (next iteration limit 4984)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits N_match=4530 sigma_overall_arcsec=0.426 sigma_q1_arcsec=0.352 sigma_q2_arcsec=0.450 sigma_q3_arcsec=0.451 sigma_q4_arcsec=0.461 n_q1=1268 n_q2=894 n_q3=1327 n_q4=1041 worst_quadrant_to_overall_ratio=1.083
The image catalog is written to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits -region wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.MEdLzjhIxe (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits' -> 'wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS-calibrated image found: wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Checking if the catalog wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS catalog name: wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=449, bad_region=0, passed=8182
Got 8182 stars (including 7721 good ones) from the SExtractor catalog wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat
util/solve_plate_with_UCAC5 got 8182 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4550 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4515 matched stars entering correct_measured_positions(), 4515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4515 matched stars entering correct_measured_positions(), 8182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4550 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4515 matched stars entering correct_measured_positions(), 8182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4515 matched stars entering correct_measured_positions(), 8182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4515 stars left (next iteration limit 4966)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits N_match=4515 sigma_overall_arcsec=0.464 sigma_q1_arcsec=0.409 sigma_q2_arcsec=0.509 sigma_q3_arcsec=0.432 sigma_q4_arcsec=0.487 n_q1=1053 n_q2=1347 n_q3=888 n_q4=1227 worst_quadrant_to_overall_ratio=1.097
The image catalog is written to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits -region wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.auvuw6XVCt (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
Checking if the catalog wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
WCS catalog name: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=321, bad_region=0, passed=6858
Got 6858 stars (including 6526 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat
util/solve_plate_with_UCAC5 got 6858 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4531 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4494 matched stars entering correct_measured_positions(), 4495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4493 matched stars entering correct_measured_positions(), 6858 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4531 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4495 matched stars entering correct_measured_positions(), 6858 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4495 matched stars entering correct_measured_positions(), 6858 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4495 stars left (next iteration limit 4942)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4495 robust_rms=9.720 arcsec worst_quadrant_rms=10.334 arcsec
SIP_REFIT: SIP order 3 trial: matched=4495 robust_rms=0.350 arcsec worst_quadrant_rms=0.364 arcsec
SIP_REFIT: SIP order 5 trial: matched=4495 robust_rms=0.284 arcsec worst_quadrant_rms=0.298 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4495 robust_rms_before=0.879 arcsec robust_rms_before_corrected=0.309 arcsec robust_rms_after=0.284 arcsec worst_quadrant_rms_before=0.347 worst_quadrant_rms_after=0.298
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:18.973 +05:58:15.68 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 6858 stars ###
'wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/correct_sextractor_wcs_catalog_usingxy2sky2088976.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.879 -> 0.284 arcsec)
WCS_QUALITY_DIAG: file=fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits N_match=4495 sigma_overall_arcsec=0.302 sigma_q1_arcsec=0.291 sigma_q2_arcsec=0.337 sigma_q3_arcsec=0.287 sigma_q4_arcsec=0.308 n_q1=1197 n_q2=1270 n_q3=1056 n_q4=972 worst_quadrant_to_overall_ratio=1.115
The image catalog is written to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits -region wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.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.MaNIxqbXEf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
Checking if the catalog wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
WCS catalog name: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=316, bad_region=0, passed=6799
Got 6799 stars (including 6480 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat
util/solve_plate_with_UCAC5 got 6799 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
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: 4486 matched stars entering correct_measured_positions(), 4486 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4486 matched stars entering correct_measured_positions(), 6798 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4522 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(), 6797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4487 matched stars entering correct_measured_positions(), 6797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4487 stars left (next iteration limit 4934)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4487 robust_rms=9.521 arcsec worst_quadrant_rms=10.223 arcsec
SIP_REFIT: SIP order 3 trial: matched=4487 robust_rms=0.344 arcsec worst_quadrant_rms=0.362 arcsec
SIP_REFIT: SIP order 5 trial: matched=4487 robust_rms=0.277 arcsec worst_quadrant_rms=0.299 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4487 robust_rms_before=0.889 arcsec robust_rms_before_corrected=0.304 arcsec robust_rms_after=0.277 arcsec worst_quadrant_rms_before=0.336 worst_quadrant_rms_after=0.299
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:16.762 +05:58:31.61 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 6799 stars ###
'wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/correct_sextractor_wcs_catalog_usingxy2sky2089080.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.889 -> 0.277 arcsec)
WCS_QUALITY_DIAG: file=fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits N_match=4487 sigma_overall_arcsec=0.294 sigma_q1_arcsec=0.292 sigma_q2_arcsec=0.337 sigma_q3_arcsec=0.282 sigma_q4_arcsec=0.291 n_q1=1217 n_q2=1303 n_q3=1058 n_q4=909 worst_quadrant_to_overall_ratio=1.145
The image catalog is written to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits -region wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits to local_wcs_cache/
'wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits' -> 'local_wcs_cache/wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits'
Saving the final (post-refit) wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits to local_wcs_cache/
'wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits' -> 'local_wcs_cache/wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits'
Saving the final (post-refit) wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits to local_wcs_cache/
'wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits' -> 'local_wcs_cache/wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits'
Saving the final (post-refit) wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits to local_wcs_cache/
'wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits' -> 'local_wcs_cache/wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits sigma_overall=0.426 worst_q_ratio=1.083
ref2=Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits sigma_overall=0.464 worst_q_ratio=1.097
new1=fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits sigma_overall=0.302 worst_q_ratio=1.115
new2=fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits sigma_overall=0.294 worst_q_ratio=1.145
reference average sigma_overall=0.445 worst_q_ratio=1.09
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300_astrometric_residuals.png (4530 matched stars from wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493_astrometric_residuals.png (4515 matched stars from wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265_astrometric_residuals.png (4495 matched stars from wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266_astrometric_residuals.png (4487 matched stars from wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits'
Saving fully-calibrated image wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits'
Preparing the HTML report for the field Peg-11-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:13:24.84 +04:45:51.4: 11.20 +/- 0.01 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:13:24.84 +04:45:51.4: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.23 +/- 0.00
Forced photometry filter REJECTED candidate at 22:13:24.84 +04:45:51.4: ref_mag=11.23 +/- 0.00 new_mean_mag=11.5080 delta=-0.28 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20905_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 20905_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
**** FOUND 22:31:14.66 +06:22:48.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20936_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 20936_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Peg-11-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
SExtractor catalog cache: saved Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.cat to cache
SExtractor catalog cache: saved Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Creating symlink local_wcs_cache/wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits exists and is non-empty
wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits exists and is non-empty
wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits exists and is non-empty
wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (1st reference image)
verification OK: wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:17:09.147 +06:00:12.37 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits (1st new image)
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:18.973 +05:58:15.68 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 22:17:18.973 +05:58:15.68
Angular distance between the image centers 0.0520 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits (2nd new image)
verification OK: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:17:16.762 +05:58:31.61 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 22:17:16.762 +05:58:31.61
Angular distance between the image centers 0.0422 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 22:17:18.973 +05:58:15.68
Second-epoch second image center 22:17:16.762 +05:58:31.61
Angular distance between the image centers 0.01018 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits &> /tmp/tmp.g9Qm0OJTr3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits &> /tmp/tmp.jAHqlF9GS7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits &> /tmp/tmp.zIh4d4LfGf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits &> /tmp/tmp.AWXZEU5vJU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
Found non-empty wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits and wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
The reference image (wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits) and catalog (wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat) found
'wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat' -> 'wcsmag.cat'
Read 49086 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2980 to 342.2142 deg, Dec +0.6967 to +11.2720 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.2980 to 342.2142 deg, Dec 0.6967 to 11.2720 deg
Loaded 6047 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4866 out of 5316 total matches.
Matched with Tycho-2 5316 out of 49086 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.420900
a=0.000000 b=1.000000 c=22.420900
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.09
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 49086 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.2980 to 342.2142 deg, Dec +0.6967 to +11.2720 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.2980 to 342.2142 deg, Dec 0.6967 to 11.2720 deg
Loaded 6047 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4866 out of 5316 total matches.
Matched with Tycho-2 5316 out of 49086 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Forced-photometry filter: calibrated wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits -> calib.txt_param_ref_wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (aperture=4.8)
Read 51877 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 326.3357 to 342.2473 deg, Dec +0.7146 to +11.2610 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 326.3357 to 342.2473 deg, Dec 0.7146 to 11.2610 deg
Loaded 6042 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4832 out of 5335 total matches.
Matched with Tycho-2 5335 out of 51877 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Forced-photometry filter: calibrated wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits -> calib.txt_param_ref_wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 58 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
2.1 pix Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
2.4 pix fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
2.4 pix fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
Limiting magnitude estimates:
15.1 mag. Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
15.2 mag. Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
15.0 mag. fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
15.0 mag. fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.3 (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.g9Qm0OJTr3 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits' -> 'wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS-calibrated image found: wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
Checking if the catalog wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits
WCS catalog name: wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=2220, bad_region=0, passed=49065
Got 49065 stars (including 46775 good ones) from the SExtractor catalog wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 49065 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4544 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4519 matched stars entering correct_measured_positions(), 4519 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4519 matched stars entering correct_measured_positions(), 49065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4544 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4518 matched stars entering correct_measured_positions(), 49065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4517 matched stars entering correct_measured_positions(), 49065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4517 stars left (next iteration limit 4970)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits N_match=4517 sigma_overall_arcsec=0.406 sigma_q1_arcsec=0.340 sigma_q2_arcsec=0.436 sigma_q3_arcsec=0.422 sigma_q4_arcsec=0.453 n_q1=1279 n_q2=891 n_q3=1277 n_q4=1070 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits -region wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.jAHqlF9GS7 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits' -> 'wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS_IMAGE_NAME=wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS-calibrated image found: wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
Checking if the catalog wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits alredy exist and is non-empty...
Catalog wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat corresponding to the image wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits
WCS catalog name: wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=2471, bad_region=0, passed=51847
Got 51847 stars (including 49304 good ones) from the SExtractor catalog wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat
util/solve_plate_with_UCAC5 got 51847 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4538 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4511 matched stars entering correct_measured_positions(), 4511 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4511 matched stars entering correct_measured_positions(), 51847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4538 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4513 matched stars entering correct_measured_positions(), 51847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4513 matched stars entering correct_measured_positions(), 51847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4513 stars left (next iteration limit 4962)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits N_match=4513 sigma_overall_arcsec=0.438 sigma_q1_arcsec=0.368 sigma_q2_arcsec=0.482 sigma_q3_arcsec=0.406 sigma_q4_arcsec=0.483 n_q1=1055 n_q2=1343 n_q3=876 n_q4=1239 worst_quadrant_to_overall_ratio=1.103
The image catalog is written to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits -region wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.zIh4d4LfGf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
Checking if the catalog wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
WCS catalog name: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1565, bad_region=20, passed=42189
Got 42189 stars (including 40537 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat
util/solve_plate_with_UCAC5 got 42189 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 4518 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4489 matched stars entering correct_measured_positions(), 4489 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4489 matched stars entering correct_measured_positions(), 42189 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 4518 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4488 matched stars entering correct_measured_positions(), 42189 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4488 matched stars entering correct_measured_positions(), 42189 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4488 stars left (next iteration limit 4937)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.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=4488 robust_rms=9.732 arcsec worst_quadrant_rms=10.329 arcsec
SIP_REFIT: SIP order 3 trial: matched=4488 robust_rms=0.343 arcsec worst_quadrant_rms=0.362 arcsec
SIP_REFIT: SIP order 5 trial: matched=4488 robust_rms=0.280 arcsec worst_quadrant_rms=0.299 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4488 robust_rms_before=0.282 arcsec robust_rms_before_corrected=0.292 arcsec robust_rms_after=0.280 arcsec worst_quadrant_rms_before=0.296 worst_quadrant_rms_after=0.299
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.296 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits N_match=4488 sigma_overall_arcsec=0.298 sigma_q1_arcsec=0.300 sigma_q2_arcsec=0.337 sigma_q3_arcsec=0.249 sigma_q4_arcsec=0.300 n_q1=1211 n_q2=1256 n_q3=1051 n_q4=970 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits -region wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.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.AWXZEU5vJU (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
WCS_IMAGE_NAME=wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
WCS-calibrated image found: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
Checking if the catalog wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat corresponding to the image wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
WCS catalog name: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1555, bad_region=26, passed=42108
Got 42108 stars (including 40469 good ones) from the SExtractor catalog wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat
util/solve_plate_with_UCAC5 got 42108 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 4509 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4480 matched stars entering correct_measured_positions(), 4480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4480 matched stars entering correct_measured_positions(), 42101 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 4509 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4478 matched stars entering correct_measured_positions(), 42101 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4478 matched stars entering correct_measured_positions(), 42101 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4478 stars left (next iteration limit 4928)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.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=4478 robust_rms=9.551 arcsec worst_quadrant_rms=10.005 arcsec
SIP_REFIT: SIP order 3 trial: matched=4478 robust_rms=0.344 arcsec worst_quadrant_rms=0.359 arcsec
SIP_REFIT: SIP order 5 trial: matched=4478 robust_rms=0.273 arcsec worst_quadrant_rms=0.293 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4478 robust_rms_before=0.274 arcsec robust_rms_before_corrected=0.294 arcsec robust_rms_after=0.273 arcsec worst_quadrant_rms_before=0.293 worst_quadrant_rms_after=0.293
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.293 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits N_match=4478 sigma_overall_arcsec=0.297 sigma_q1_arcsec=0.308 sigma_q2_arcsec=0.313 sigma_q3_arcsec=0.267 sigma_q4_arcsec=0.286 n_q1=1221 n_q2=1293 n_q3=1059 n_q4=905 worst_quadrant_to_overall_ratio=1.057
The image catalog is written to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits -region wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-51-32_20.00sec_-0.00C_LIGHTs_0265.fits
Saving fully-calibrated image wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Peg-11-Q1b1x1_035316_TTUQ1b1x1_2060319_A2tY86ns/wcs_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266.fits
Preparing the HTML report for the field Peg-11-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:02:44.64 +08:29:45.5: 13.15 +/- 0.04 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:38:00.05 +07:52:37.9: 14.11 +/- 0.08 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:52:39.88 +08:45:24.5: 12.61 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:00:41.42 +10:33:06.3: 14.25 +/- 0.11 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:39:29.82 +07:10:28.5: 10.00 +/- 0.00 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:42:34.43 +01:15:14.4: 14.28 +/- 0.12 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:26:28.64 +10:55:21.4: 14.67 +/- 0.14 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:46:29.95 +07:09:23.6: 13.59 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:46:33.87 +04:57:19.4: 14.35 +/- 0.12 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:24:56.79 +09:24:19.5: 12.84 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:38:00.05 +07:52:37.9: 13.88 +/- 0.07 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:52:39.88 +08:45:24.5: 12.63 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:26:28.64 +10:55:21.4: 14.57 +/- 0.12 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:24:56.79 +09:24:19.5: 12.82 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:39:29.82 +07:10:28.5: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 22:39:29.82 +07:10:28.5: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:02:44.64 +08:29:45.5: 13.16 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:00:41.42 +10:33:06.3: 14.19 +/- 0.08 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:42:34.43 +01:15:14.4: 14.16 +/- 0.11 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:46:29.95 +07:09:23.6: 13.52 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:46:33.87 +04:57:19.4: 14.08 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
Forced photometry reference-image weighted average: 13.97 +/- 0.05
Forced photometry reference-image weighted average: 14.62 +/- 0.09
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Forced photometry reference-image weighted average: 13.16 +/- 0.03
Forced photometry reference-image weighted average: 14.21 +/- 0.07
Forced photometry reference-image weighted average: 14.22 +/- 0.08
Forced photometry reference-image weighted average: 13.56 +/- 0.04
Forced photometry reference-image weighted average: 14.19 +/- 0.08
Forced photometry filter REJECTED candidate at 21:52:39.88 +08:45:24.5: ref_mag=12.62 +/- 0.02 new_mean_mag=12.4701 delta=0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:38:00.05 +07:52:37.9: ref_mag=13.97 +/- 0.05 new_mean_mag=14.0505 delta=-0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:26:28.64 +10:55:21.4: ref_mag=14.62 +/- 0.09 new_mean_mag=14.5929 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:24:56.79 +09:24:19.5: ref_mag=12.83 +/- 0.02 new_mean_mag=13.1105 delta=-0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:02:44.64 +08:29:45.5: ref_mag=13.16 +/- 0.03 new_mean_mag=13.1034 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:00:41.42 +10:33:06.3: ref_mag=14.21 +/- 0.07 new_mean_mag=13.9518 delta=0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:42:34.43 +01:15:14.4: ref_mag=14.22 +/- 0.08 new_mean_mag=14.2628 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:46:29.95 +07:09:23.6: ref_mag=13.56 +/- 0.04 new_mean_mag=13.8148 delta=-0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:46:33.87 +04:57:19.4: ref_mag=14.19 +/- 0.08 new_mean_mag=14.3625 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:49:56.28 +05:12:52.1: 12.36 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:12:18.49 +02:45:16.1: 13.71 +/- 0.07 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:42:55.98 +01:10:16.8: 14.42 +/- 0.14 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:45:37.94 +10:16:26.3: 12.78 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:38:27.71 +03:26:46.1: 12.90 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:04:46.10 +10:31:51.3: 15.60 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 21:50:34.22 +10:56:04.2: 13.47 +/- 0.07 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:47:17.39 +10:27:28.1: 14.78 +/- 0.19 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:38:21.09 +09:15:38.0: 13.98 +/- 0.09 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:46:13.94 +01:17:17.3: 14.75 +/- 0.19 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:12:18.49 +02:45:16.1: 13.68 +/- 0.06 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:04:46.10 +10:31:51.3: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:42:55.98 +01:10:16.8: 14.08 +/- 0.11 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:50:34.22 +10:56:04.2: 13.76 +/- 0.07 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 21:49:56.28 +05:12:52.1: 12.48 +/- 0.02 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:45:37.94 +10:16:26.3: 12.68 +/- 0.03 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:38:27.71 +03:26:46.1: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.05
Forced photometry filter REJECTED candidate at 22:12:18.49 +02:45:16.1: ref_mag=13.69 +/- 0.05 new_mean_mag=13.6368 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 14.20 +/- 0.09
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:38:21.09 +09:15:38.0: 13.77 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.05
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:47:17.39 +10:27:28.1: 14.12 +/- 0.11 detection
Forced photometry filter REJECTED candidate at 22:42:55.98 +01:10:16.8: ref_mag=14.20 +/- 0.09 new_mean_mag=14.1061 delta=0.10 (need > 0.90)
Forced photometry reference-image weighted average: 12.42 +/- 0.02
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Forced photometry filter REJECTED candidate at 21:50:34.22 +10:56:04.2: ref_mag=13.61 +/- 0.05 new_mean_mag=13.5113 delta=0.10 (need > 0.90)
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Forced photometry filter REJECTED candidate at 21:49:56.28 +05:12:52.1: ref_mag=12.42 +/- 0.02 new_mean_mag=13.1815 delta=-0.76 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:45:37.94 +10:16:26.3: ref_mag=12.73 +/- 0.02 new_mean_mag=13.1575 delta=-0.43 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:38:27.71 +03:26:46.1: ref_mag=12.75 +/- 0.02 new_mean_mag=12.8575 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 13.85 +/- 0.06
Forced photometry reference-image weighted average: 14.28 +/- 0.09
Forced photometry filter REJECTED candidate at 22:38:21.09 +09:15:38.0: ref_mag=13.85 +/- 0.06 new_mean_mag=13.9751 delta=-0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:47:17.39 +10:27:28.1: ref_mag=14.28 +/- 0.09 new_mean_mag=14.4415 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:46:13.94 +01:17:17.3: 14.60 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.67 +/- 0.13
Forced photometry filter REJECTED candidate at 22:46:13.94 +01:17:17.3: ref_mag=14.67 +/- 0.13 new_mean_mag=14.2740 delta=0.40 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:40:28.36 +03:40:33.3: 14.93 +/- 0.20 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:46:52.12 +04:53:05.3: 14.46 +/- 0.13 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:48:13.19 +06:59:49.9: 14.48 +/- 0.13 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:34:23.83 +03:44:31.6: 14.66 +/- 0.15 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:41:00.49 +01:29:48.4: 14.73 +/- 0.18 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:41:46.44 +01:11:52.7: 14.74 +/- 0.18 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:42:50.28 +01:21:00.4: 14.60 +/- 0.16 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:35:53.64 +04:29:30.9: 14.78 +/- 0.16 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:37:05.39 +01:45:38.4: 14.58 +/- 0.15 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:40:28.36 +03:40:33.3: 14.72 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.13
Forced photometry filter REJECTED candidate at 22:40:28.36 +03:40:33.3: ref_mag=14.81 +/- 0.13 new_mean_mag=14.5113 delta=0.30 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:46:52.12 +04:53:05.3: 14.46 +/- 0.14 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:48:13.19 +06:59:49.9: 14.71 +/- 0.18 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:34:23.83 +03:44:31.6: 14.57 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.10
Forced photometry reference-image weighted average: 14.56 +/- 0.11
Forced photometry filter REJECTED candidate at 22:46:52.12 +04:53:05.3: ref_mag=14.46 +/- 0.10 new_mean_mag=14.5191 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:41:46.44 +01:11:52.7: 14.52 +/- 0.16 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:41:00.49 +01:29:48.4: 14.89 +/- 0.21 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:42:50.28 +01:21:00.4: 14.48 +/- 0.16 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:35:53.64 +04:29:30.9: 14.47 +/- 0.11 detection
Forced photometry filter REJECTED candidate at 22:48:13.19 +06:59:49.9: ref_mag=14.56 +/- 0.11 new_mean_mag=14.4689 delta=0.09 (need > 0.90)
Forced photometry reference-image weighted average: 14.62 +/- 0.11
Forced photometry filter REJECTED candidate at 22:34:23.83 +03:44:31.6: ref_mag=14.62 +/- 0.11 new_mean_mag=14.2648 delta=0.35 (need > 0.90)
Forced photometry reference-image weighted average: 14.80 +/- 0.14
Forced photometry reference-image weighted average: 14.62 +/- 0.12
Forced photometry reference-image weighted average: 14.58 +/- 0.09
Forced photometry reference-image weighted average: 14.54 +/- 0.11
Forced photometry filter REJECTED candidate at 22:41:00.49 +01:29:48.4: ref_mag=14.80 +/- 0.14 new_mean_mag=14.3777 delta=0.42 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:35:53.64 +04:29:30.9: ref_mag=14.58 +/- 0.09 new_mean_mag=14.4678 delta=0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:41:46.44 +01:11:52.7: ref_mag=14.62 +/- 0.12 new_mean_mag=14.3843 delta=0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:42:50.28 +01:21:00.4: ref_mag=14.54 +/- 0.11 new_mean_mag=14.4728 delta=0.07 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:37:05.39 +01:45:38.4: 14.41 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.49 +/- 0.10
Forced photometry filter REJECTED candidate at 22:37:05.39 +01:45:38.4: ref_mag=14.49 +/- 0.10 new_mean_mag=14.3341 delta=0.15 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:46:59.63 +07:20:53.6: 14.35 +/- 0.12 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:46:43.87 +01:16:07.2: 14.67 +/- 0.19 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:47:36.64 +06:24:24.7: 14.78 +/- 0.18 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:40:45.61 +10:16:31.8: 15.03 +/- 0.22 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:47:58.99 +09:27:14.0: 14.20 +/- 0.10 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:42:49.22 +10:35:33.9: 14.12 +/- 0.10 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:44:28.00 +02:01:31.3: 14.61 +/- 0.16 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:44:39.94 +01:01:40.7: 14.80 +/- 0.20 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:38:52.24 +08:20:29.0: 14.58 +/- 0.14 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:46:59.63 +07:20:53.6: 14.22 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.08
Forced photometry filter REJECTED candidate at 22:46:59.63 +07:20:53.6: ref_mag=14.28 +/- 0.08 new_mean_mag=14.5826 delta=-0.30 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:46:43.87 +01:16:07.2: 14.57 +/- 0.18 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:47:36.64 +06:24:24.7: 14.66 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.13
Forced photometry filter REJECTED candidate at 22:46:43.87 +01:16:07.2: ref_mag=14.62 +/- 0.13 new_mean_mag=14.5834 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.72 +/- 0.12
Forced photometry filter REJECTED candidate at 22:47:36.64 +06:24:24.7: ref_mag=14.72 +/- 0.12 new_mean_mag=14.6035 delta=0.11 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:47:58.99 +09:27:14.0: 14.25 +/- 0.12 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:40:45.61 +10:16:31.8: 14.83 +/- 0.18 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:44:39.94 +01:01:40.7: 14.90 +/- 0.23 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:42:49.22 +10:35:33.9: 14.30 +/- 0.11 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:44:28.00 +02:01:31.3: 14.39 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.08
Forced photometry reference-image weighted average: 14.91 +/- 0.14
Forced photometry filter REJECTED candidate at 22:47:58.99 +09:27:14.0: ref_mag=14.22 +/- 0.08 new_mean_mag=14.5379 delta=-0.31 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:40:45.61 +10:16:31.8: ref_mag=14.91 +/- 0.14 new_mean_mag=14.6718 delta=0.24 (need > 0.90)
Forced photometry reference-image weighted average: 14.20 +/- 0.07
Forced photometry reference-image weighted average: 14.84 +/- 0.15
Forced photometry reference-image weighted average: 14.49 +/- 0.11
Forced photometry filter REJECTED candidate at 22:42:49.22 +10:35:33.9: ref_mag=14.20 +/- 0.07 new_mean_mag=14.5152 delta=-0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:44:39.94 +01:01:40.7: ref_mag=14.84 +/- 0.15 new_mean_mag=14.5428 delta=0.30 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:44:28.00 +02:01:31.3: ref_mag=14.49 +/- 0.11 new_mean_mag=14.4048 delta=0.08 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:38:52.24 +08:20:29.0: 14.44 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.50 +/- 0.10
Forced photometry filter REJECTED candidate at 22:38:52.24 +08:20:29.0: ref_mag=14.50 +/- 0.10 new_mean_mag=14.5599 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:44:46.77 +01:29:00.9: 15.22 +/- 0.29 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:36:22.81 +06:26:42.5: 14.65 +/- 0.13 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:44:21.50 +01:32:47.5: 14.93 +/- 0.22 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:36:54.84 +01:25:03.5: 14.61 +/- 0.14 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:45:45.36 +01:26:33.6: 15.38 +/- 0.34 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:32:26.26 +01:34:43.6: 14.33 +/- 0.12 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:42:57.24 +05:37:23.3: 14.80 +/- 0.17 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:41:05.44 +01:03:29.1: 14.76 +/- 0.19 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:44:35.41 +01:40:44.2: 14.93 +/- 0.23 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:44:46.77 +01:29:00.9: 14.97 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.18
Forced photometry filter REJECTED candidate at 22:44:46.77 +01:29:00.9: ref_mag=15.08 +/- 0.18 new_mean_mag=14.5301 delta=0.55 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:36:22.81 +06:26:42.5: 14.38 +/- 0.11 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:44:21.50 +01:32:47.5: 14.86 +/- 0.23 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:45:45.36 +01:26:33.6: 14.81 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.49 +/- 0.08
Forced photometry filter REJECTED candidate at 22:36:22.81 +06:26:42.5: ref_mag=14.49 +/- 0.08 new_mean_mag=14.4485 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.90 +/- 0.16
Forced photometry reference-image weighted average: 14.98 +/- 0.18
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:32:26.26 +01:34:43.6: 14.28 +/- 0.12 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:41:05.44 +01:03:29.1: 14.57 +/- 0.18 detection
Forced photometry filter REJECTED candidate at 22:44:21.50 +01:32:47.5: ref_mag=14.90 +/- 0.16 new_mean_mag=14.6444 delta=0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:45:45.36 +01:26:33.6: ref_mag=14.98 +/- 0.18 new_mean_mag=14.4265 delta=0.55 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:42:57.24 +05:37:23.3: 14.94 +/- 0.20 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:36:54.84 +01:25:03.5: 14.80 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.09
Forced photometry reference-image weighted average: 14.66 +/- 0.13
Forced photometry reference-image weighted average: 14.86 +/- 0.13
Forced photometry filter REJECTED candidate at 22:32:26.26 +01:34:43.6: ref_mag=14.30 +/- 0.09 new_mean_mag=14.4608 delta=-0.16 (need > 0.90)
Forced photometry reference-image weighted average: 14.69 +/- 0.11
Forced photometry filter REJECTED candidate at 22:41:05.44 +01:03:29.1: ref_mag=14.66 +/- 0.13 new_mean_mag=14.4654 delta=0.19 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:42:57.24 +05:37:23.3: ref_mag=14.86 +/- 0.13 new_mean_mag=14.6489 delta=0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:36:54.84 +01:25:03.5: ref_mag=14.69 +/- 0.11 new_mean_mag=14.5023 delta=0.19 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:44:35.41 +01:40:44.2: 15.04 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.18
Forced photometry filter REJECTED candidate at 22:44:35.41 +01:40:44.2: ref_mag=14.98 +/- 0.18 new_mean_mag=14.6695 delta=0.31 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:44:50.85 +01:22:54.5: 14.73 +/- 0.19 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:02:16.25 +10:33:59.3: 14.87 +/- 0.19 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:12:12.34 +09:46:35.5: 14.96 +/- 0.19 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:07:44.20 +08:40:08.2: 14.85 +/- 0.17 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:11:10.01 +09:27:31.0: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:19:35.36 +01:10:31.2: 14.99 +/- 0.20 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:36:11.31 +01:44:09.4: 14.61 +/- 0.15 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-18_02-54-38_20.00sec_4.90C_LIGHT_0300.fits at 22:04:12.20 +10:04:22.5: 14.55 +/- 0.14 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:44:50.85 +01:22:54.5: 14.43 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.55 +/- 0.12
Forced photometry filter REJECTED candidate at 22:44:50.85 +01:22:54.5: ref_mag=14.55 +/- 0.12 new_mean_mag=14.6072 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:19:35.36 +01:10:31.2: 14.99 +/- 0.19 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:02:16.25 +10:33:59.3: 14.60 +/- 0.12 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:36:11.31 +01:44:09.4: 14.68 +/- 0.16 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:12:12.34 +09:46:35.5: 14.99 +/- 0.17 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:11:10.01 +09:27:31.0: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:07:44.20 +08:40:08.2: 14.95 +/- 0.16 detection
Forced photometry on wcs_Peg-11-Q1b1x1_2026-07-20_05-30-58_20.00sec_4.90C_LIGHT_0493.fits at 22:04:12.20 +10:04:22.5: 14.64 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.14
Forced photometry reference-image weighted average: 14.68 +/- 0.10
Forced photometry filter REJECTED candidate at 22:19:35.36 +01:10:31.2: ref_mag=14.99 +/- 0.14 new_mean_mag=14.5424 delta=0.45 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:02:16.25 +10:33:59.3: ref_mag=14.68 +/- 0.10 new_mean_mag=14.2862 delta=0.39 (need > 0.90)
Forced photometry reference-image weighted average: 14.97 +/- 0.13
Forced photometry reference-image weighted average: 14.64 +/- 0.11
Forced photometry reference-image weighted average: 14.90 +/- 0.12
Forced photometry reference-image weighted average: 14.60 +/- 0.09
Forced photometry filter REJECTED candidate at 22:12:12.34 +09:46:35.5: ref_mag=14.97 +/- 0.13 new_mean_mag=14.6547 delta=0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:36:11.31 +01:44:09.4: ref_mag=14.64 +/- 0.11 new_mean_mag=14.6388 delta=0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:07:44.20 +08:40:08.2: ref_mag=14.90 +/- 0.12 new_mean_mag=14.4409 delta=0.46 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:04:12.20 +10:04:22.5: ref_mag=14.60 +/- 0.09 new_mean_mag=14.4851 delta=0.11 (need > 0.90)
Adding exclusion_list_local.txt__out56539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57613.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 56195_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 56195_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 56200_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 56200_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56202_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 56202_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56203_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 56203_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56206_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 56206_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 56208_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 56208_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 56209_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 56209_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56210_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 56210_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56211_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 56211_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56212_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 56212_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 56539_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
Preparing report for the candidate 56539_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
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Considering the candidate 56559_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 56559_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 56597_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 56597_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 56928_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 56928_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 56970_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 56970_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57029_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57029_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57075_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57075_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57077_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57077_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57081_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57081_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
**** FOUND 22:19:34.54 +09:06:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57197_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57197_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57223_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57223_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57274_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57274_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57283_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57283_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57289_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57289_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57292_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57292_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57314_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57314_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57328_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57328_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57329_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57329_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57332_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57332_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57334_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57334_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57337_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57337_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57352_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57352_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57358_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57358_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57368_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57368_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57375_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57375_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57388_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57388_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57393_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57393_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57400_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57400_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57403_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57403_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57405_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57405_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57414_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57414_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57433_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57433_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57439_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57439_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57441_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57441_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57443_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57443_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57444_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57444_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57465_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57465_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57466_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57466_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57474_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57474_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57527_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57527_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57575_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57575_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57613_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
Preparing report for the candidate 57613_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
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Considering the candidate 57687_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57687_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57748_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57748_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57782_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57782_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 57786_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 57786_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
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Considering the candidate 24406_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 24406_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks
**** FOUND 22:31:14.65 +06:22:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36115_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266
The candidate 36115_fd_Peg-11-Q1b1x1_2026-09-06_03-52-31_20.00sec_-0.00C_LIGHTs_0266 did not pass the final checks