This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ
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 07 31.4016 2461252.9016 12.39 00:09:08.31 +20:37:08.6
109.74266 -41.16687 galactic Peg Second-epoch detections are separated by 0.5" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.71 Niobe -1 -0 1 12.5 0 0
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:09:08.31 +20:37:08.6: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:09:08.31 +20:37:08.6: 16.11 +/- 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,2461252.9016,12.39,0.05,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 20260731.4016 12.39CV 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 07 31.4016 2461252.9016 13.12 00:08:48.13 +21:29:12.0
109.88934 -40.30284 galactic Peg Second-epoch detections are separated by 1.0" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.695 Bella -1 -0 1 12.9 -0 0
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:08:48.13 +21:29:12.0: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:08:48.13 +21:29:12.0: 15.91 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.91 +/- 0.29
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,2461252.9016,13.12,0.05,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 20260731.4016 13.12CV 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 07 31.4016 2461252.9016 13.70 00:09:40.97 +17:21:49.3
108.93249 -44.37008 galactic Peg Second-epoch detections are separated by 2.3" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.665 Sabine -1 -1 1 14.0 -0 -0
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:09:40.97 +17:21:49.3: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:09:40.97 +17:21:49.3: 15.90 +/- 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,2461252.9016,13.70,0.05,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 20260731.4016 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.62147831 09.01.2026 02:54:45.726 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
First image: 2461049.62147831 09.01.2026 02:54:45.726 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Last image: 2461252.90194880 31.07.2026 09:38:38.376 /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
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: 2 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): 8592
Objects passed selection criteria: 8560
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 6631.5
Average stars matched: 6496 (97.9567 %)
Memory usage VmPeak: 241036 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 31 04:44:31 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.62147831 09.01.2026 02:54:45.726 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
First image: 2461049.62147831 09.01.2026 02:54:45.726 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Last image: 2461252.90194880 31.07.2026 09:38:38.376 /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 23
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 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): 50768
Objects passed selection criteria: 50648
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 41344.2
Average stars matched: 40287.8 (97.4446 %)
Memory usage VmPeak: 272156 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jul 31 04:45:16 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
SExtractor catalog cache: saved Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.cat to cache
SExtractor catalog cache: saved Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.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-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.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: 2461252.90127898
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-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits exists and is non-empty
Saving wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits to local_wcs_cache/
'wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits' -> 'local_wcs_cache/wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits'
wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits exists and is non-empty
Saving wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits to local_wcs_cache/
'wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits' -> 'local_wcs_cache/wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits'
wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits exists and is non-empty
Saving wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits to local_wcs_cache/
'wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits' -> 'local_wcs_cache/wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits'
wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits exists and is non-empty
Saving wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits to local_wcs_cache/
'wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits' -> 'local_wcs_cache/wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits (1st reference image)
verification OK: wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Image size: 941.5'x626.9' 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: 00:00:00.348 +21:59:54.97 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits (1st new image)
verification OK: wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
Image size: 941.1'x626.6' 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: 23:59:47.668 +22:00:22.12 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.348 +21:59:54.97
Second-epoch image center 23:59:47.668 +22:00:22.12
Angular distance between the image centers 0.0496 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits (2nd new image)
verification OK: wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
Image size: 941.1'x626.6' 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: 23:59:44.838 +21:59:41.74 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.348 +21:59:54.97
Second-epoch image center 23:59:44.838 +21:59:41.74
Angular distance between the image centers 0.0600 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 23:59:47.668 +22:00:22.12
Second-epoch second image center 23:59:44.838 +21:59:41.74
Angular distance between the image centers 0.01566 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-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits &> /tmp/tmp.lIrQv0t6Jn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits &> /tmp/tmp.B4toZZkv4q
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits &> /tmp/tmp.qiznbH4Vi2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits &> /tmp/tmp.e099lai3Oa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat
Found non-empty wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat
The reference image (wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits) and catalog (wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat) found
'wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 9019 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.2902 to 8.8792 deg, Dec +16.5101 to +27.2962 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 351.2902 to 8.8792 deg, Dec 16.5101 to 27.2962 deg
Loaded 6920 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): 5313 out of 5630 total matches.
Matched with Tycho-2 5630 out of 9019 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.881100
a=0.000000 b=1.000000 c=22.881100
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.27
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.27
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 9019 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.2902 to 8.8792 deg, Dec +16.5101 to +27.2962 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 351.2902 to 8.8792 deg, Dec 16.5101 to 27.2962 deg
Loaded 6920 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): 5313 out of 5630 total matches.
Matched with Tycho-2 5630 out of 9019 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Forced-photometry filter: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits -> calib.txt_param_ref_wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits (aperture=5.9)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 8998 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.2893 to 8.8790 deg, Dec +16.5101 to +27.2944 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 351.2893 to 8.8790 deg, Dec 16.5101 to 27.2944 deg
Loaded 6921 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): 5335 out of 5642 total matches.
Matched with Tycho-2 5642 out of 8998 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
Forced-photometry filter: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits -> calib.txt_param_ref_wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
2.0 pix Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
2.4 pix fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
2.4 pix fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
Limiting magnitude estimates:
15.3 mag. Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
15.3 mag. Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
14.2 mag. fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
14.2 mag. fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.lIrQv0t6Jn (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits' -> 'wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Checking if the catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
WCS catalog name: wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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=673, bad_region=0, passed=9019
Got 9019 stars (including 8339 good ones) from the SExtractor catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat
util/solve_plate_with_UCAC5 got 9019 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2902 through 0 to 8.8792, gap 8.8792 to 351.2902
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 4906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 9019 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
RA wraps around 0/360 boundary: field RA 351.2896 through 0 to 8.8800, gap 8.8800 to 351.2896
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 9019 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 9019 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4909 stars left (next iteration limit 5396)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits N_match=4909 sigma_overall_arcsec=0.297 sigma_q1_arcsec=0.399 sigma_q2_arcsec=0.281 sigma_q3_arcsec=0.278 sigma_q4_arcsec=0.245 n_q1=1233 n_q2=1314 n_q3=1161 n_q4=1201 worst_quadrant_to_overall_ratio=1.344
The image catalog is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits -region wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.B4toZZkv4q (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.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-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits' -> 'wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.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-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
WCS-calibrated image found: wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
Checking if the catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
WCS catalog name: wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.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=657, bad_region=0, passed=8998
Got 8998 stars (including 8327 good ones) from the SExtractor catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat
util/solve_plate_with_UCAC5 got 8998 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2893 through 0 to 8.8790, gap 8.8790 to 351.2893
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 4909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 8998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2887 through 0 to 8.8798, gap 8.8798 to 351.2887
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 8998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 8998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4912 stars left (next iteration limit 5399)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits N_match=4912 sigma_overall_arcsec=0.280 sigma_q1_arcsec=0.369 sigma_q2_arcsec=0.268 sigma_q3_arcsec=0.259 sigma_q4_arcsec=0.240 n_q1=1238 n_q2=1312 n_q3=1162 n_q4=1200 worst_quadrant_to_overall_ratio=1.318
The image catalog is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits -region wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qiznbH4Vi2 (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_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.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_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
Checking if the catalog wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
WCS catalog name: wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.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=362, bad_region=0, passed=4343
Got 4343 stars (including 3972 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat
util/solve_plate_with_UCAC5 got 4343 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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
RA wraps around 0/360 boundary: field RA 351.4454 through 0 to 9.0283, gap 9.0283 to 351.4454
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 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 3912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3904 matched stars entering correct_measured_positions(), 3904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3904 matched stars entering correct_measured_positions(), 4343 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.4450 through 0 to 9.0292, gap 9.0292 to 351.4450
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 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 3911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3903 matched stars entering correct_measured_positions(), 4343 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 3903 matched stars entering correct_measured_positions(), 4343 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 3903 stars left (next iteration limit 4294)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3903 robust_rms=11.384 arcsec worst_quadrant_rms=12.456 arcsec
SIP_REFIT: SIP order 3 trial: matched=3903 robust_rms=0.423 arcsec worst_quadrant_rms=0.434 arcsec
SIP_REFIT: SIP order 5 trial: matched=3903 robust_rms=0.290 arcsec worst_quadrant_rms=0.304 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3903 robust_rms_before=0.936 arcsec robust_rms_before_corrected=0.315 arcsec robust_rms_after=0.290 arcsec worst_quadrant_rms_before=0.327 worst_quadrant_rms_after=0.304
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.327 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits N_match=3903 sigma_overall_arcsec=0.323 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.339 sigma_q3_arcsec=0.313 sigma_q4_arcsec=0.327 n_q1=1000 n_q2=897 n_q3=1045 n_q4=961 worst_quadrant_to_overall_ratio=1.048
The image catalog is written to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits -region wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.e099lai3Oa (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_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.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_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
Checking if the catalog wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
WCS catalog name: wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.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=354, bad_region=0, passed=4317
Got 4317 stars (including 3957 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat
util/solve_plate_with_UCAC5 got 4317 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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
RA wraps around 0/360 boundary: field RA 351.4318 through 0 to 8.9284, gap 8.9284 to 351.4318
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 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 3893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3885 matched stars entering correct_measured_positions(), 3885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3885 matched stars entering correct_measured_positions(), 4317 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.4316 through 0 to 8.9291, gap 8.9291 to 351.4316
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 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 3893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3885 matched stars entering correct_measured_positions(), 4317 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 3885 matched stars entering correct_measured_positions(), 4317 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 3885 stars left (next iteration limit 4273)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3885 robust_rms=11.163 arcsec worst_quadrant_rms=12.592 arcsec
SIP_REFIT: SIP order 3 trial: matched=3885 robust_rms=0.406 arcsec worst_quadrant_rms=0.417 arcsec
SIP_REFIT: SIP order 5 trial: matched=3885 robust_rms=0.289 arcsec worst_quadrant_rms=0.301 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3885 robust_rms_before=0.924 arcsec robust_rms_before_corrected=0.311 arcsec robust_rms_after=0.289 arcsec worst_quadrant_rms_before=0.319 worst_quadrant_rms_after=0.301
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.319 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits N_match=3885 sigma_overall_arcsec=0.321 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.332 sigma_q3_arcsec=0.302 sigma_q4_arcsec=0.340 n_q1=1017 n_q2=869 n_q3=1040 n_q4=959 worst_quadrant_to_overall_ratio=1.061
The image catalog is written to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits -region wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits sigma_overall=0.297 worst_q_ratio=1.344
ref2=Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits sigma_overall=0.280 worst_q_ratio=1.318
new1=fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits sigma_overall=0.323 worst_q_ratio=1.048
new2=fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits sigma_overall=0.321 worst_q_ratio=1.061
reference average sigma_overall=0.2885 worst_q_ratio=1.331
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067_astrometric_residuals.png (4909 matched stars from wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068_astrometric_residuals.png (4912 matched stars from wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302_astrometric_residuals.png (3903 matched stars from wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303_astrometric_residuals.png (3885 matched stars from wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits'
Saving fully-calibrated image wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits'
Preparing the HTML report for the field Peg-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Peg-04-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-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
SExtractor catalog cache: saved Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.cat to cache
SExtractor catalog cache: saved Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.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-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Creating symlink local_wcs_cache/wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits exists and is non-empty
wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits exists and is non-empty
wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits exists and is non-empty
wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits (1st reference image)
verification OK: wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Image size: 941.5'x626.9' 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: 00:00:00.348 +21:59:54.97 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits (1st new image)
verification OK: wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
Image size: 941.1'x626.6' 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: 23:59:47.668 +22:00:22.12 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.348 +21:59:54.97
Second-epoch image center 23:59:47.668 +22:00:22.12
Angular distance between the image centers 0.0496 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits (2nd new image)
verification OK: wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
Image size: 941.1'x626.6' 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: 23:59:44.838 +21:59:41.74 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.348 +21:59:54.97
Second-epoch image center 23:59:44.838 +21:59:41.74
Angular distance between the image centers 0.0600 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 23:59:47.668 +22:00:22.12
Second-epoch second image center 23:59:44.838 +21:59:41.74
Angular distance between the image centers 0.01566 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-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits &> /tmp/tmp.8MIS00afuq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits &> /tmp/tmp.wrEGeoWaOP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits &> /tmp/tmp.n6a8PcRYeo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits &> /tmp/tmp.ePRN9WnkOh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat
Found non-empty wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat
The reference image (wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits) and catalog (wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat) found
'wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 54563 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.2893 to 8.8872 deg, Dec +16.4838 to +27.3003 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 351.2893 to 8.8872 deg, Dec 16.4838 to 27.3003 deg
Loaded 6940 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): 5095 out of 5798 total matches.
Matched with Tycho-2 5798 out of 54563 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.777100
a=0.000000 b=1.000000 c=22.777100
From vast_summary.log: estimated ref. image limiting mag.: -7.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 54563 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.2893 to 8.8872 deg, Dec +16.4838 to +27.3003 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 351.2893 to 8.8872 deg, Dec 16.4838 to 27.3003 deg
Loaded 6940 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): 5095 out of 5798 total matches.
Matched with Tycho-2 5798 out of 54563 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Forced-photometry filter: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits -> calib.txt_param_ref_wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits (aperture=4.7)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 54021 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.2769 to 8.8790 deg, Dec +16.4843 to +27.2989 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 351.2769 to 8.8790 deg, Dec 16.4843 to 27.2989 deg
Loaded 6948 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): 5113 out of 5797 total matches.
Matched with Tycho-2 5797 out of 54021 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
Forced-photometry filter: calibrated wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits -> calib.txt_param_ref_wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 21 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
1.9 pix Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
2.3 pix fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
2.3 pix fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
Limiting magnitude estimates:
15.4 mag. Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
15.4 mag. Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
14.4 mag. fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
14.4 mag. fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.8 (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.8MIS00afuq (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits' -> 'wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
Checking if the catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits
WCS catalog name: wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.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=2723, bad_region=3, passed=54549
Got 54549 stars (including 51710 good ones) from the SExtractor catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat
util/solve_plate_with_UCAC5 got 54549 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2893 through 0 to 8.8872, gap 8.8872 to 351.2893
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 4910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 54549 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
RA wraps around 0/360 boundary: field RA 351.2887 through 0 to 8.8880, gap 8.8880 to 351.2887
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 54549 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 54549 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4910 stars left (next iteration limit 5401)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits N_match=4910 sigma_overall_arcsec=0.285 sigma_q1_arcsec=0.379 sigma_q2_arcsec=0.270 sigma_q3_arcsec=0.268 sigma_q4_arcsec=0.241 n_q1=1203 n_q2=1321 n_q3=1164 n_q4=1222 worst_quadrant_to_overall_ratio=1.331
The image catalog is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits -region wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.wrEGeoWaOP (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.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-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits' -> 'wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.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-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
WCS-calibrated image found: wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
Checking if the catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat corresponding to the image wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits
WCS catalog name: wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=2675, bad_region=3, passed=54003
Got 54003 stars (including 51231 good ones) from the SExtractor catalog wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat
util/solve_plate_with_UCAC5 got 54003 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2769 through 0 to 8.8790, gap 8.8790 to 351.2769
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 4906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 54003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2763 through 0 to 8.8798, gap 8.8798 to 351.2763
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 54003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 54003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4907 stars left (next iteration limit 5396)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits N_match=4907 sigma_overall_arcsec=0.265 sigma_q1_arcsec=0.354 sigma_q2_arcsec=0.252 sigma_q3_arcsec=0.244 sigma_q4_arcsec=0.227 n_q1=1190 n_q2=1317 n_q3=1184 n_q4=1216 worst_quadrant_to_overall_ratio=1.335
The image catalog is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits -region wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.n6a8PcRYeo (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_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.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_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
Checking if the catalog wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
WCS catalog name: wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=929, bad_region=1, passed=28931
Got 28931 stars (including 27946 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat
util/solve_plate_with_UCAC5 got 28931 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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
RA wraps around 0/360 boundary: field RA 351.4336 through 0 to 9.0350, gap 9.0350 to 351.4336
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 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 4911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 28931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.4334 through 0 to 9.0360, gap 9.0360 to 351.4334
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 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 28931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 28931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4911 stars left (next iteration limit 5402)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits N_match=4911 sigma_overall_arcsec=0.319 sigma_q1_arcsec=0.321 sigma_q2_arcsec=0.329 sigma_q3_arcsec=0.308 sigma_q4_arcsec=0.320 n_q1=1215 n_q2=1132 n_q3=1339 n_q4=1225 worst_quadrant_to_overall_ratio=1.034
The image catalog is written to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits -region wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ePRN9WnkOh (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_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.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_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
Checking if the catalog wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
WCS catalog name: wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.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=6, blended=964, bad_region=1, passed=28881
Got 28881 stars (including 27867 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat
util/solve_plate_with_UCAC5 got 28881 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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
RA wraps around 0/360 boundary: field RA 351.4245 through 0 to 9.0331, gap 9.0331 to 351.4245
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 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 4910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 28881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.4245 through 0 to 9.0339, gap 9.0339 to 351.4245
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 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 28881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 28881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4911 stars left (next iteration limit 5401)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits N_match=4911 sigma_overall_arcsec=0.318 sigma_q1_arcsec=0.321 sigma_q2_arcsec=0.329 sigma_q3_arcsec=0.303 sigma_q4_arcsec=0.327 n_q1=1213 n_q2=1130 n_q3=1345 n_q4=1223 worst_quadrant_to_overall_ratio=1.036
The image catalog is written to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits -region wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.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_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-37-40_20.00sec_-0.00C_LIGHTs_0302.fits
Saving fully-calibrated image wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.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_2026-07-31_CI_Peg-04-Q1b1x1_044100_TTUQ1b1x1_2113285_ee1hZQGQ/wcs_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303.fits
Preparing the HTML report for the field Peg-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:56:08.24 +20:06:26.6: 13.40 +/- 0.03 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:44:59.81 +24:06:51.1: 11.15 +/- 0.00 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:44:13.66 +20:38:14.0: 12.59 +/- 0.02 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:45:56.73 +26:58:45.3: 13.31 +/- 0.03 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:31:33.70 +20:50:54.4: 12.64 +/- 0.02 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:58:09.04 +24:19:46.5: 12.92 +/- 0.02 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:09:08.31 +20:37:08.6: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:57:52.34 +25:06:30.7: 12.59 +/- 0.02 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:08:48.13 +21:29:12.0: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:37:14.75 +22:14:55.8: 13.18 +/- 0.03 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:45:56.73 +26:58:45.3: 13.28 +/- 0.03 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:09:08.31 +20:37:08.6: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:44:59.81 +24:06:51.1: 11.15 +/- 0.00 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:31:33.70 +20:50:54.4: 12.68 +/- 0.02 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:44:13.66 +20:38:14.0: 12.58 +/- 0.02 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:58:09.04 +24:19:46.5: 12.89 +/- 0.02 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:57:52.34 +25:06:30.7: 12.60 +/- 0.02 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:56:08.24 +20:06:26.6: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry reference-image weighted average: 11.15 +/- 0.00
Forced photometry filter REJECTED candidate at 23:45:56.73 +26:58:45.3: ref_mag=13.30 +/- 0.02 new_mean_mag=13.6240 delta=-0.33 (need > 0.90)
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry filter REJECTED candidate at 00:31:33.70 +20:50:54.4: ref_mag=12.66 +/- 0.02 new_mean_mag=12.6406 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:44:59.81 +24:06:51.1: ref_mag=11.15 +/- 0.00 new_mean_mag=11.2541 delta=-0.10 (need > 0.90)
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter REJECTED candidate at 23:44:13.66 +20:38:14.0: ref_mag=12.59 +/- 0.01 new_mean_mag=12.6521 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:56:08.24 +20:06:26.6: ref_mag=13.44 +/- 0.02 new_mean_mag=13.6044 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:57:52.34 +25:06:30.7: ref_mag=12.59 +/- 0.01 new_mean_mag=12.5968 delta=-0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:58:09.04 +24:19:46.5: ref_mag=12.90 +/- 0.02 new_mean_mag=12.9946 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:08:48.13 +21:29:12.0: 15.91 +/- 0.29 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:37:14.75 +22:14:55.8: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 15.91 +/- 0.29
Forced photometry filter KEPT candidate at 00:08:48.13 +21:29:12.0: ref_mag=15.91 +/- 0.29 new_mean_mag=13.1144 delta=2.79 (need > 0.90)
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter REJECTED candidate at 23:37:14.75 +22:14:55.8: ref_mag=13.22 +/- 0.02 new_mean_mag=13.2815 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:44:57.92 +21:22:28.8: 13.48 +/- 0.04 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:09:07.61 +21:03:44.1: 13.35 +/- 0.03 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:51:35.89 +24:17:56.6: 13.96 +/- 0.06 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:50:15.28 +23:47:31.1: 13.61 +/- 0.04 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:39:22.69 +24:43:44.4: 13.54 +/- 0.04 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 23:59:58.52 +25:52:52.3: 13.32 +/- 0.04 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:09:40.97 +17:21:49.3: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-54-45_20.00sec_-15.00C_LIGHT_0067.fits at 00:18:25.22 +26:07:49.4: 13.57 +/- 0.05 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:59:58.52 +25:52:52.3: 13.25 +/- 0.03 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:39:22.69 +24:43:44.4: 13.58 +/- 0.05 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:09:07.61 +21:03:44.1: 13.32 +/- 0.03 detection
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:51:35.89 +24:17:56.6: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:50:15.28 +23:47:31.1: 13.63 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 23:59:58.52 +25:52:52.3: ref_mag=13.28 +/- 0.02 new_mean_mag=13.5719 delta=-0.29 (need > 0.90)
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 23:44:57.92 +21:22:28.8: 13.53 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 23:39:22.69 +24:43:44.4: ref_mag=13.56 +/- 0.03 new_mean_mag=13.5966 delta=-0.04 (need > 0.90)
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:09:40.97 +17:21:49.3: 15.90 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 00:09:07.61 +21:03:44.1: ref_mag=13.33 +/- 0.02 new_mean_mag=13.4467 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter REJECTED candidate at 23:51:35.89 +24:17:56.6: ref_mag=13.94 +/- 0.04 new_mean_mag=13.9472 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:50:15.28 +23:47:31.1: ref_mag=13.62 +/- 0.03 new_mean_mag=13.7135 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Forced photometry filter REJECTED candidate at 23:44:57.92 +21:22:28.8: ref_mag=13.50 +/- 0.03 new_mean_mag=13.5331 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Peg-04-Q1b1x1_2026-01-08_20-55-35_20.00sec_-14.90C_LIGHT_0068.fits at 00:18:25.22 +26:07:49.4: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Forced photometry filter REJECTED candidate at 00:18:25.22 +26:07:49.4: ref_mag=13.59 +/- 0.04 new_mean_mag=13.7888 delta=-0.20 (need > 0.90)
Adding exclusion_list_local.txt__out68248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68562.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68067_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68067_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68068_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68068_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68070_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68070_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68071_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68071_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68248_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
Preparing report for the candidate 68248_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68267_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68267_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68297_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68297_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68299_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68299_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
**** FOUND 23:52:30.05 +21:41:07.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68316_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68316_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
**** FOUND 00:27:28.11 +26:18:16.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68343_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68343_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68426_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
Preparing report for the candidate 68426_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68427_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68427_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68471_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68471_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68507_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68507_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68529_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68529_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68562_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
Preparing report for the candidate 68562_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68564_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68564_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68569_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68569_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68625_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68625_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68626_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 68626_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04721_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303
The candidate 04721_fd_Peg-04-Q1b1x1_2026-07-31_04-38-38_20.00sec_0.00C_LIGHTs_0303 did not pass the final checks