This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki
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 08 17.3479 2461269.8479 12.18 00:01:34.37 +22:43:26.4
108.14828 -38.71204 galactic Peg Second-epoch detections are separated by 0.3" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.71 Niobe -0 0 0 12.3 0 0
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:01:34.37 +22:43:26.4: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:01:34.37 +22:43:26.4: 15.95 +/- 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,2461269.8479,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260817.3479 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3479 2461269.8479 12.61 00:09:24.77 +24:31:18.6
110.88395 -37.36479 galactic Peg Second-epoch detections are separated by 0.7" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.695 Bella -0 0 0 12.5 -0 0
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:09:24.77 +24:31:18.6: 15.90 +/- 0.34 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:09:24.77 +24:31:18.6: 16.04 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.90 +/- 0.34
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,2461269.8479,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260817.3479 12.61CV 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 08 17.3479 2461269.8479 13.76 00:04:27.93 +18:39:56.3
107.69306 -42.81191 galactic Peg Second-epoch detections are separated by 0.6" and 10.4 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 -0 1 13.8 -0 0
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:04:27.93 +18:39:56.3: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:04:27.93 +18:39:56.3: 16.06 +/- 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,2461269.8479,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260817.3479 13.76CV 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: 2461238.93300359 17.07.2026 10:23:21.510 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
First image: 2461238.93300359 17.07.2026 10:23:21.510 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
Last image: 2461269.84827951 17.08.2026 08:21:21.350 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 7240
Objects passed selection criteria: 7238
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 7017.75
Average stars matched: 6699.5 (95.4651 %)
Memory usage VmPeak: 233748 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 17 03:42:48 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: 2461238.93300359 17.07.2026 10:23:21.510 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
First image: 2461238.93300359 17.07.2026 10:23:21.510 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
Last image: 2461269.84827951 17.08.2026 08:21:21.350 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 82
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.14
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: 21 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): 43743
Objects passed selection criteria: 43635
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 42560.8
Average stars matched: 40327 (94.7516 %)
Memory usage VmPeak: 266020 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 17 03:43:57 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
SExtractor catalog cache: saved Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.cat to cache
SExtractor catalog cache: saved Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.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-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.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: 2461269.84757786
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-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits exists and is non-empty
wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits exists and is non-empty
wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits exists and is non-empty
wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits (1st reference image)
verification OK: wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.055 +22:00:03.17 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits (1st new image)
verification OK: wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:01.085 +21:59:56.70 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.055 +22:00:03.17
Second-epoch image center 00:00:01.085 +21:59:56.70
Angular distance between the image centers 0.0044 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits (2nd new image)
verification OK: wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:03.385 +22:00:48.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.055 +22:00:03.17
Second-epoch image center 00:00:03.385 +22:00:48.62
Angular distance between the image centers 0.0180 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 00:00:01.085 +21:59:56.70
Second-epoch second image center 00:00:03.385 +22:00:48.62
Angular distance between the image centers 0.01694 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-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits &> /tmp/tmp.SXLPt6B1FM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits &> /tmp/tmp.GZSPIJevca
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits &> /tmp/tmp.H7turbFeT7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits &> /tmp/tmp.tPsP2d2CBZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.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-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits and wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.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-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits and wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat
Found non-empty wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits and wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat
The reference image (wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits) and catalog (wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat) found
'wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 8496 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.2292 to 8.6895 deg, Dec +16.5741 to +27.2661 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 351.2292 to 8.6895 deg, Dec 16.5741 to 27.2661 deg
Loaded 6834 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): 5352 out of 5532 total matches.
Matched with Tycho-2 5532 out of 8496 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.546900
a=0.000000 b=1.000000 c=22.546900
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.14
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.14
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 8496 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.2292 to 8.6895 deg, Dec +16.5741 to +27.2661 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 351.2292 to 8.6895 deg, Dec 16.5741 to 27.2661 deg
Loaded 6834 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): 5352 out of 5532 total matches.
Matched with Tycho-2 5532 out of 8496 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
Forced-photometry filter: calibrated wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits -> calib.txt_param_ref_wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits (aperture=6.2)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 9308 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.1747 to 8.6909 deg, Dec +16.5687 to +27.2687 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 351.1747 to 8.6909 deg, Dec 16.5687 to 27.2687 deg
Loaded 6863 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): 5389 out of 5623 total matches.
Matched with Tycho-2 5623 out of 9308 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
Forced-photometry filter: calibrated wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits -> calib.txt_param_ref_wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
2.3 pix Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
2.2 pix fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
2.2 pix fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
Limiting magnitude estimates:
15.1 mag. Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
15.3 mag. Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
15.3 mag. fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
15.3 mag. fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.SXLPt6B1FM (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_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.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-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits' -> 'wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.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-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
WCS_IMAGE_NAME=wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
WCS-calibrated image found: wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
Checking if the catalog wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits alredy exist and is non-empty...
Catalog wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
WCS catalog name: wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=487, bad_region=1919, passed=8496
Got 8496 stars (including 6185 good ones) from the SExtractor catalog wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat
util/solve_plate_with_UCAC5 got 8496 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2292 through 0 to 8.6895, gap 8.6895 to 351.2292
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 16.6 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: 4907 matched stars entering correct_measured_positions(), 4907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 6972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2294 through 0 to 8.6895, gap 8.6895 to 351.2294
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 16.6 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: 4907 matched stars entering correct_measured_positions(), 6972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 6972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4907 stars left (next iteration limit 5397)
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-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits N_match=4907 sigma_overall_arcsec=0.381 sigma_q1_arcsec=0.318 sigma_q2_arcsec=0.395 sigma_q3_arcsec=0.451 sigma_q4_arcsec=0.370 n_q1=1541 n_q2=833 n_q3=1634 n_q4=899 worst_quadrant_to_overall_ratio=1.184
The image catalog is written to wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits -region wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_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.GZSPIJevca (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_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.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-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits' -> 'wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.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-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
WCS_IMAGE_NAME=wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
WCS-calibrated image found: wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
Checking if the catalog wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat corresponding to the image wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits alredy exist and is non-empty...
Catalog wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat corresponding to the image wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
WCS catalog name: wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=597, bad_region=2092, passed=9308
Got 9308 stars (including 6731 good ones) from the SExtractor catalog wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat
util/solve_plate_with_UCAC5 got 9308 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.1747 through 0 to 8.6909, gap 8.6909 to 351.1747
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 16.6 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: 4910 matched stars entering correct_measured_positions(), 4910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 7647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.1749 through 0 to 8.6909, gap 8.6909 to 351.1749
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 16.6 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
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 7647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 7647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4910 stars left (next iteration limit 5401)
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-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits N_match=4910 sigma_overall_arcsec=0.395 sigma_q1_arcsec=0.341 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.441 sigma_q4_arcsec=0.396 n_q1=1557 n_q2=835 n_q3=1623 n_q4=895 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits -region wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.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.H7turbFeT7 (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_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.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_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
Checking if the catalog wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
WCS catalog name: wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=582, bad_region=2100, passed=9341
Got 9341 stars (including 6767 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat
util/solve_plate_with_UCAC5 got 9341 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2590 through 0 to 8.7373, gap 8.7373 to 351.2590
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 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 7662 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 351.2580 through 0 to 8.7375, gap 8.7375 to 351.2580
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 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 7662 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 7662 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4905 stars left (next iteration limit 5391)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4905 robust_rms=6.619 arcsec worst_quadrant_rms=10.141 arcsec
SIP_REFIT: SIP order 3 trial: matched=4905 robust_rms=0.462 arcsec worst_quadrant_rms=0.591 arcsec
SIP_REFIT: SIP order 5 trial: matched=4905 robust_rms=0.327 arcsec worst_quadrant_rms=0.375 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4905 robust_rms_before=0.894 arcsec robust_rms_before_corrected=0.334 arcsec robust_rms_after=0.327 arcsec worst_quadrant_rms_before=0.378 worst_quadrant_rms_after=0.375
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.378 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits N_match=4905 sigma_overall_arcsec=0.348 sigma_q1_arcsec=0.293 sigma_q2_arcsec=0.346 sigma_q3_arcsec=0.411 sigma_q4_arcsec=0.337 n_q1=1543 n_q2=838 n_q3=1628 n_q4=896 worst_quadrant_to_overall_ratio=1.183
The image catalog is written to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits -region wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.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.tPsP2d2CBZ (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_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.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_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
Checking if the catalog wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
WCS catalog name: wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=589, bad_region=2100, passed=9283
Got 9283 stars (including 6710 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat
util/solve_plate_with_UCAC5 got 9283 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2589 through 0 to 8.7382, gap 8.7382 to 351.2589
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 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 4905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 7603 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2579 through 0 to 8.7383, gap 8.7383 to 351.2579
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 16.6 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: 4907 matched stars entering correct_measured_positions(), 7603 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 7603 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4907 stars left (next iteration limit 5395)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4907 robust_rms=6.616 arcsec worst_quadrant_rms=9.938 arcsec
SIP_REFIT: SIP order 3 trial: matched=4907 robust_rms=0.498 arcsec worst_quadrant_rms=0.604 arcsec
SIP_REFIT: SIP order 5 trial: matched=4907 robust_rms=0.362 arcsec worst_quadrant_rms=0.394 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4907 robust_rms_before=0.913 arcsec robust_rms_before_corrected=0.365 arcsec robust_rms_after=0.362 arcsec worst_quadrant_rms_before=0.398 worst_quadrant_rms_after=0.394
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.398 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits N_match=4907 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.321 sigma_q2_arcsec=0.413 sigma_q3_arcsec=0.425 sigma_q4_arcsec=0.357 n_q1=1545 n_q2=844 n_q3=1629 n_q4=889 worst_quadrant_to_overall_ratio=1.126
The image catalog is written to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits -region wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits to local_wcs_cache/
'wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits' -> 'local_wcs_cache/wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits'
Saving the final (post-refit) wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits to local_wcs_cache/
'wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits' -> 'local_wcs_cache/wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits'
Saving the final (post-refit) wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits to local_wcs_cache/
'wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits' -> 'local_wcs_cache/wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits'
Saving the final (post-refit) wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits to local_wcs_cache/
'wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits' -> 'local_wcs_cache/wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits sigma_overall=0.381 worst_q_ratio=1.184
ref2=Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits sigma_overall=0.395 worst_q_ratio=1.116
new1=fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits sigma_overall=0.348 worst_q_ratio=1.183
new2=fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits sigma_overall=0.378 worst_q_ratio=1.126
reference average sigma_overall=0.388 worst_q_ratio=1.15
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302_astrometric_residuals.png (4907 matched stars from wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930_astrometric_residuals.png (4910 matched stars from wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380_astrometric_residuals.png (4905 matched stars from wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381_astrometric_residuals.png (4907 matched stars from wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits'
Saving fully-calibrated image wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits'
Preparing the HTML report for the field Peg-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:01:34.37 +22:43:26.4: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:01:34.37 +22:43:26.4: 15.95 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20796.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20796_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
Preparing report for the candidate 20796_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Peg-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:01:34.37 +22:43:26.4
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
SExtractor catalog cache: saved Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.cat to cache
SExtractor catalog cache: saved Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.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-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
Creating symlink local_wcs_cache/wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits exists and is non-empty
wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits exists and is non-empty
wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits exists and is non-empty
wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits (1st reference image)
verification OK: wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.055 +22:00:03.17 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits (1st new image)
verification OK: wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:01.085 +21:59:56.70 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.055 +22:00:03.17
Second-epoch image center 00:00:01.085 +21:59:56.70
Angular distance between the image centers 0.0044 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits (2nd new image)
verification OK: wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:03.385 +22:00:48.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.055 +22:00:03.17
Second-epoch image center 00:00:03.385 +22:00:48.62
Angular distance between the image centers 0.0180 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 00:00:01.085 +21:59:56.70
Second-epoch second image center 00:00:03.385 +22:00:48.62
Angular distance between the image centers 0.01694 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-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits &> /tmp/tmp.ruNwIcL3vZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits &> /tmp/tmp.ONCqrKqRxs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits &> /tmp/tmp.fb4QZE0fDa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits &> /tmp/tmp.0CWNEgTaBo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.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-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits and wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.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-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits and wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat
Found non-empty wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits and wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat
The reference image (wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits) and catalog (wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat) found
'wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 49884 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.1954 to 8.7302 deg, Dec +16.5689 to +27.2662 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 351.1954 to 8.7302 deg, Dec 16.5689 to 27.2662 deg
Loaded 6874 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): 5205 out of 5737 total matches.
Matched with Tycho-2 5737 out of 49884 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.424700
a=0.000000 b=1.000000 c=22.424700
From vast_summary.log: estimated ref. image limiting mag.: -7.14
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
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 49884 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.1954 to 8.7302 deg, Dec +16.5689 to +27.2662 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 351.1954 to 8.7302 deg, Dec 16.5689 to 27.2662 deg
Loaded 6874 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): 5205 out of 5737 total matches.
Matched with Tycho-2 5737 out of 49884 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
Forced-photometry filter: calibrated wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits -> calib.txt_param_ref_wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits (aperture=4.8)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 52523 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.1747 to 8.6934 deg, Dec +16.5638 to +27.2712 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 351.1747 to 8.6934 deg, Dec 16.5638 to 27.2712 deg
Loaded 6866 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): 5145 out of 5746 total matches.
Matched with Tycho-2 5746 out of 52523 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
Forced-photometry filter: calibrated wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits -> calib.txt_param_ref_wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 42 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
2.1 pix Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
2.1 pix fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
2.1 pix fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
Limiting magnitude estimates:
15.3 mag. Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
15.4 mag. Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
15.4 mag. fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
15.4 mag. fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ruNwIcL3vZ (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_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.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-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits' -> 'wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.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-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
WCS_IMAGE_NAME=wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
WCS-calibrated image found: wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
Checking if the catalog wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits alredy exist and is non-empty...
Catalog wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat corresponding to the image wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits
WCS catalog name: wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=2460, bad_region=8934, passed=49871
Got 49871 stars (including 38903 good ones) from the SExtractor catalog wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat
util/solve_plate_with_UCAC5 got 49871 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.1954 through 0 to 8.7302, gap 8.7302 to 351.1954
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 16.6 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 43184 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.1956 through 0 to 8.7302, gap 8.7302 to 351.1956
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 16.6 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: 4906 matched stars entering correct_measured_positions(), 43184 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 43184 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4906 stars left (next iteration limit 5396)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits N_match=4906 sigma_overall_arcsec=0.368 sigma_q1_arcsec=0.315 sigma_q2_arcsec=0.377 sigma_q3_arcsec=0.438 sigma_q4_arcsec=0.360 n_q1=1575 n_q2=842 n_q3=1614 n_q4=875 worst_quadrant_to_overall_ratio=1.192
The image catalog is written to wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits -region wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_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.ONCqrKqRxs (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_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.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-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits' -> 'wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.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-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
WCS_IMAGE_NAME=wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
WCS-calibrated image found: wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
Checking if the catalog wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat corresponding to the image wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits alredy exist and is non-empty...
Catalog wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat corresponding to the image wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits
WCS catalog name: wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=2681, bad_region=9176, passed=52502
Got 52502 stars (including 41075 good ones) from the SExtractor catalog wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat
util/solve_plate_with_UCAC5 got 52502 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.1747 through 0 to 8.6934, gap 8.6934 to 351.1747
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 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 4905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 45670 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.1750 through 0 to 8.6934, gap 8.6934 to 351.1750
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 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 45670 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 45670 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4905 stars left (next iteration limit 5395)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits N_match=4905 sigma_overall_arcsec=0.383 sigma_q1_arcsec=0.338 sigma_q2_arcsec=0.381 sigma_q3_arcsec=0.428 sigma_q4_arcsec=0.386 n_q1=1582 n_q2=843 n_q3=1595 n_q4=885 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits -region wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.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.fb4QZE0fDa (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_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.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_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
Checking if the catalog wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
WCS catalog name: wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=2652, bad_region=9609, passed=53038
Got 53038 stars (including 41225 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat
util/solve_plate_with_UCAC5 got 53038 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2305 through 0 to 8.7531, gap 8.7531 to 351.2305
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 16.6 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: 4904 matched stars entering correct_measured_positions(), 4904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 45804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 351.2295 through 0 to 8.7533, gap 8.7533 to 351.2295
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 16.6 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: 4904 matched stars entering correct_measured_positions(), 45804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 45804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4904 stars left (next iteration limit 5394)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4904 robust_rms=6.689 arcsec worst_quadrant_rms=9.723 arcsec
SIP_REFIT: SIP order 3 trial: matched=4904 robust_rms=0.458 arcsec worst_quadrant_rms=0.589 arcsec
SIP_REFIT: SIP order 5 trial: matched=4904 robust_rms=0.319 arcsec worst_quadrant_rms=0.374 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4904 robust_rms_before=0.876 arcsec robust_rms_before_corrected=0.325 arcsec robust_rms_after=0.319 arcsec worst_quadrant_rms_before=0.374 worst_quadrant_rms_after=0.374
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.374 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits N_match=4904 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.296 sigma_q2_arcsec=0.336 sigma_q3_arcsec=0.409 sigma_q4_arcsec=0.322 n_q1=1581 n_q2=854 n_q3=1584 n_q4=885 worst_quadrant_to_overall_ratio=1.203
The image catalog is written to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits -region wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.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.0CWNEgTaBo (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_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.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_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
Checking if the catalog wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
WCS catalog name: wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=2668, bad_region=9595, passed=53198
Got 53198 stars (including 41378 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat
util/solve_plate_with_UCAC5 got 53198 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2306 through 0 to 8.7556, gap 8.7556 to 351.2306
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 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4903 matched stars entering correct_measured_positions(), 4903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4903 matched stars entering correct_measured_positions(), 45957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.2296 through 0 to 8.7557, gap 8.7557 to 351.2296
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 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4903 matched stars entering correct_measured_positions(), 45957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4903 matched stars entering correct_measured_positions(), 45957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4903 stars left (next iteration limit 5393)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4903 robust_rms=6.670 arcsec worst_quadrant_rms=9.563 arcsec
SIP_REFIT: SIP order 3 trial: matched=4903 robust_rms=0.495 arcsec worst_quadrant_rms=0.599 arcsec
SIP_REFIT: SIP order 5 trial: matched=4903 robust_rms=0.357 arcsec worst_quadrant_rms=0.389 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4903 robust_rms_before=0.896 arcsec robust_rms_before_corrected=0.358 arcsec robust_rms_after=0.357 arcsec worst_quadrant_rms_before=0.388 worst_quadrant_rms_after=0.389
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.388 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits N_match=4903 sigma_overall_arcsec=0.373 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.386 sigma_q3_arcsec=0.415 sigma_q4_arcsec=0.357 n_q1=1570 n_q2=860 n_q3=1589 n_q4=884 worst_quadrant_to_overall_ratio=1.112
The image catalog is written to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits -region wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.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-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.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_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-20-20_20.00sec_-0.00C_LIGHT_0380.fits
Saving fully-calibrated image wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.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_2026-08-17_CI_Peg-04-Q2b1x1_034025_TTUQ2b1x1_2374200_hDxNIMki/wcs_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381.fits
Preparing the HTML report for the field Peg-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:31:15.62 +23:12:35.0: 14.62 +/- 0.14 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:57:47.16 +19:46:01.2: 14.46 +/- 0.10 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:06:05.13 +25:59:07.1: 13.85 +/- 0.06 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:16:17.36 +23:28:04.2: 14.67 +/- 0.12 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:08:46.07 +22:03:11.9: 15.04 +/- 0.15 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:51:06.50 +23:32:15.9: 14.68 +/- 0.11 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:57:32.16 +24:07:19.4: 14.68 +/- 0.12 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:12:16.74 +17:54:08.5: 15.43 +/- 0.24 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:35:57.60 +22:11:02.5: 14.58 +/- 0.12 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:46:58.75 +24:45:06.3: 14.73 +/- 0.13 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:51:06.50 +23:32:15.9: 14.95 +/- 0.13 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:31:15.62 +23:12:35.0: 14.61 +/- 0.12 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:12:16.74 +17:54:08.5: 15.22 +/- 0.18 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:46:58.75 +24:45:06.3: 14.81 +/- 0.12 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:16:17.36 +23:28:04.2: 14.66 +/- 0.10 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:08:46.07 +22:03:11.9: 14.77 +/- 0.11 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:57:32.16 +24:07:19.4: 14.86 +/- 0.13 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:57:47.16 +19:46:01.2: 14.42 +/- 0.08 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:35:57.60 +22:11:02.5: 14.75 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.09
Forced photometry reference-image weighted average: 14.80 +/- 0.09
Forced photometry reference-image weighted average: 15.30 +/- 0.14
Forced photometry reference-image weighted average: 14.77 +/- 0.09
Forced photometry filter REJECTED candidate at 23:31:15.62 +23:12:35.0: ref_mag=14.61 +/- 0.09 new_mean_mag=14.4892 delta=0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:51:06.50 +23:32:15.9: ref_mag=14.80 +/- 0.09 new_mean_mag=14.7891 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 14.67 +/- 0.08
Forced photometry reference-image weighted average: 14.86 +/- 0.09
Forced photometry filter REJECTED candidate at 00:12:16.74 +17:54:08.5: ref_mag=15.30 +/- 0.14 new_mean_mag=14.8240 delta=0.48 (need > 0.90)
Forced photometry reference-image weighted average: 14.76 +/- 0.09
Forced photometry reference-image weighted average: 14.44 +/- 0.06
Forced photometry filter REJECTED candidate at 23:46:58.75 +24:45:06.3: ref_mag=14.77 +/- 0.09 new_mean_mag=14.7749 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:16:17.36 +23:28:04.2: ref_mag=14.67 +/- 0.08 new_mean_mag=14.7190 delta=-0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:08:46.07 +22:03:11.9: ref_mag=14.86 +/- 0.09 new_mean_mag=14.7412 delta=0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:57:32.16 +24:07:19.4: ref_mag=14.76 +/- 0.09 new_mean_mag=14.8722 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:57:47.16 +19:46:01.2: ref_mag=14.44 +/- 0.06 new_mean_mag=14.6606 delta=-0.22 (need > 0.90)
Forced photometry reference-image weighted average: 14.66 +/- 0.09
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:06:05.13 +25:59:07.1: 13.78 +/- 0.05 detection
Forced photometry filter REJECTED candidate at 23:35:57.60 +22:11:02.5: ref_mag=14.66 +/- 0.09 new_mean_mag=14.5378 delta=0.12 (need > 0.90)
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry filter REJECTED candidate at 00:06:05.13 +25:59:07.1: ref_mag=13.81 +/- 0.04 new_mean_mag=13.9798 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:55:41.30 +18:22:55.0: 13.07 +/- 0.03 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:04:27.93 +18:39:56.3: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:42:45.57 +24:50:29.7: 14.78 +/- 0.14 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:09:24.77 +24:31:18.6: 15.90 +/- 0.34 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:15:47.06 +21:19:50.6: 10.36 +/- 0.00 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:49:23.14 +23:25:12.8: 14.32 +/- 0.10 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:15:56.34 +25:26:32.7: 13.00 +/- 0.03 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:59:13.52 +18:19:41.9: 14.80 +/- 0.13 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:34:59.00 +26:01:08.5: 15.07 +/- 0.20 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:33:45.52 +25:47:10.3: 14.81 +/- 0.17 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:59:13.52 +18:19:41.9: 14.65 +/- 0.10 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:49:23.14 +23:25:12.8: 14.45 +/- 0.10 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:55:41.30 +18:22:55.0: 13.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.08
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:04:27.93 +18:39:56.3: 16.06 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 23:59:13.52 +18:19:41.9: ref_mag=14.71 +/- 0.08 new_mean_mag=14.5803 delta=0.13 (need > 0.90)
Forced photometry reference-image weighted average: 14.39 +/- 0.07
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter REJECTED candidate at 23:49:23.14 +23:25:12.8: ref_mag=14.39 +/- 0.07 new_mean_mag=14.4863 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:15:56.34 +25:26:32.7: 13.00 +/- 0.02 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:15:47.06 +21:19:50.6: 10.40 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 23:55:41.30 +18:22:55.0: ref_mag=13.04 +/- 0.02 new_mean_mag=13.2148 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:42:45.57 +24:50:29.7: 14.79 +/- 0.13 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:09:24.77 +24:31:18.6: 16.04 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry reference-image weighted average: 10.38 +/- 0.00
Forced photometry filter REJECTED candidate at 00:15:56.34 +25:26:32.7: ref_mag=13.00 +/- 0.02 new_mean_mag=13.2939 delta=-0.30 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:15:47.06 +21:19:50.6: ref_mag=10.38 +/- 0.00 new_mean_mag=10.3762 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 14.79 +/- 0.09
Forced photometry reference-image weighted average: 15.90 +/- 0.34
Forced photometry filter REJECTED candidate at 23:42:45.57 +24:50:29.7: ref_mag=14.79 +/- 0.09 new_mean_mag=14.5589 delta=0.23 (need > 0.90)
Forced photometry filter KEPT candidate at 00:09:24.77 +24:31:18.6: ref_mag=15.90 +/- 0.34 new_mean_mag=12.6021 delta=3.30 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:34:59.00 +26:01:08.5: 15.19 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.15
Forced photometry filter REJECTED candidate at 23:34:59.00 +26:01:08.5: ref_mag=15.13 +/- 0.15 new_mean_mag=14.5976 delta=0.53 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:33:45.52 +25:47:10.3: 14.80 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.11
Forced photometry filter REJECTED candidate at 23:33:45.52 +25:47:10.3: ref_mag=14.81 +/- 0.11 new_mean_mag=14.5264 delta=0.28 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:33:20.69 +25:04:44.1: 14.93 +/- 0.18 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:14:13.88 +25:10:04.4: 14.92 +/- 0.14 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:39:27.19 +19:58:03.2: 14.81 +/- 0.15 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:39:02.80 +25:09:37.1: 15.03 +/- 0.19 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:40:18.61 +22:30:58.8: 15.10 +/- 0.20 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:34:40.96 +19:11:43.2: 14.89 +/- 0.18 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:08:22.91 +17:45:37.8: 15.13 +/- 0.18 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:33:49.79 +21:06:52.1: 15.25 +/- 0.22 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:33:20.69 +25:04:44.1: 15.07 +/- 0.18 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:14:13.88 +25:10:04.4: 14.84 +/- 0.12 detection
Forced photometry reference-image weighted average: 15.00 +/- 0.13
Forced photometry filter REJECTED candidate at 23:33:20.69 +25:04:44.1: ref_mag=15.00 +/- 0.13 new_mean_mag=14.6970 delta=0.30 (need > 0.90)
Forced photometry reference-image weighted average: 14.88 +/- 0.09
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:39:27.19 +19:58:03.2: 14.99 +/- 0.16 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:39:02.80 +25:09:37.1: 15.24 +/- 0.20 detection
Forced photometry filter REJECTED candidate at 00:14:13.88 +25:10:04.4: ref_mag=14.88 +/- 0.09 new_mean_mag=14.5725 delta=0.30 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:40:18.61 +22:30:58.8: 14.83 +/- 0.14 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:34:40.96 +19:11:43.2: 14.86 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.89 +/- 0.11
Forced photometry reference-image weighted average: 15.13 +/- 0.14
Forced photometry filter REJECTED candidate at 23:39:27.19 +19:58:03.2: ref_mag=14.89 +/- 0.11 new_mean_mag=14.6624 delta=0.23 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:08:22.91 +17:45:37.8: 15.01 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.11
Forced photometry filter REJECTED candidate at 23:39:02.80 +25:09:37.1: ref_mag=15.13 +/- 0.14 new_mean_mag=14.7304 delta=0.40 (need > 0.90)
Forced photometry reference-image weighted average: 14.87 +/- 0.12
Forced photometry filter REJECTED candidate at 23:40:18.61 +22:30:58.8: ref_mag=14.92 +/- 0.11 new_mean_mag=14.7936 delta=0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:34:40.96 +19:11:43.2: ref_mag=14.87 +/- 0.12 new_mean_mag=14.7300 delta=0.14 (need > 0.90)
Forced photometry reference-image weighted average: 15.06 +/- 0.12
Forced photometry filter REJECTED candidate at 00:08:22.91 +17:45:37.8: ref_mag=15.06 +/- 0.12 new_mean_mag=14.8355 delta=0.22 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:33:49.79 +21:06:52.1: 14.72 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.11
Forced photometry filter REJECTED candidate at 23:33:49.79 +21:06:52.1: ref_mag=14.84 +/- 0.11 new_mean_mag=14.7347 delta=0.11 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:08:51.99 +20:28:44.3: 15.29 +/- 0.20 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:18:41.13 +25:35:53.6: 15.61 +/- 0.29 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:43:36.45 +22:14:12.6: 14.71 +/- 0.12 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:33:40.49 +19:11:15.0: 15.30 +/- 0.25 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:35:25.92 +22:41:03.0: 14.91 +/- 0.17 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:36:37.36 +18:25:27.3: 14.82 +/- 0.16 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:32:56.95 +19:11:13.7: 15.09 +/- 0.22 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:33:42.16 +20:15:25.5: 14.87 +/- 0.17 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:18:41.13 +25:35:53.6: 15.53 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.57 +/- 0.19
Forced photometry filter REJECTED candidate at 00:18:41.13 +25:35:53.6: ref_mag=15.57 +/- 0.19 new_mean_mag=14.8191 delta=0.75 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:08:51.99 +20:28:44.3: 14.93 +/- 0.13 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.11
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:43:36.45 +22:14:12.6: 14.75 +/- 0.12 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:33:40.49 +19:11:15.0: 15.07 +/- 0.19 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:32:56.95 +19:11:13.7: 15.14 +/- 0.20 detection
Forced photometry filter REJECTED candidate at 00:08:51.99 +20:28:44.3: ref_mag=15.04 +/- 0.11 new_mean_mag=14.8586 delta=0.18 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:35:25.92 +22:41:03.0: 15.17 +/- 0.20 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:36:37.36 +18:25:27.3: 15.05 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.73 +/- 0.08
Forced photometry reference-image weighted average: 15.15 +/- 0.15
Forced photometry reference-image weighted average: 15.12 +/- 0.15
Forced photometry reference-image weighted average: 15.02 +/- 0.13
Forced photometry filter REJECTED candidate at 23:43:36.45 +22:14:12.6: ref_mag=14.73 +/- 0.08 new_mean_mag=14.7896 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:33:40.49 +19:11:15.0: ref_mag=15.15 +/- 0.15 new_mean_mag=14.9148 delta=0.24 (need > 0.90)
Forced photometry reference-image weighted average: 14.93 +/- 0.12
Forced photometry filter REJECTED candidate at 23:32:56.95 +19:11:13.7: ref_mag=15.12 +/- 0.15 new_mean_mag=14.9112 delta=0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:35:25.92 +22:41:03.0: ref_mag=15.02 +/- 0.13 new_mean_mag=14.8129 delta=0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:36:37.36 +18:25:27.3: ref_mag=14.93 +/- 0.12 new_mean_mag=14.7575 delta=0.17 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:33:42.16 +20:15:25.5: 14.82 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.11
Forced photometry filter REJECTED candidate at 23:33:42.16 +20:15:25.5: ref_mag=14.84 +/- 0.11 new_mean_mag=14.8929 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:34:01.66 +23:04:53.8: 14.97 +/- 0.18 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:38:27.16 +24:53:56.0: 14.84 +/- 0.15 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:17:45.02 +23:51:35.7: 15.40 +/- 0.23 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:35:42.94 +20:17:19.6: 14.67 +/- 0.13 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:34:10.65 +25:14:22.7: 15.16 +/- 0.23 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:38:27.16 +24:53:56.0: 15.03 +/- 0.17 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:35:42.94 +20:17:19.6: 14.95 +/- 0.16 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:17:45.02 +23:51:35.7: 15.22 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.11
Forced photometry reference-image weighted average: 14.78 +/- 0.10
Forced photometry filter REJECTED candidate at 23:38:27.16 +24:53:56.0: ref_mag=14.92 +/- 0.11 new_mean_mag=14.8081 delta=0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:35:42.94 +20:17:19.6: ref_mag=14.78 +/- 0.10 new_mean_mag=14.8202 delta=-0.04 (need > 0.90)
Forced photometry reference-image weighted average: 15.28 +/- 0.14
Forced photometry filter REJECTED candidate at 00:17:45.02 +23:51:35.7: ref_mag=15.28 +/- 0.14 new_mean_mag=14.8580 delta=0.43 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:34:01.66 +23:04:53.8: 15.00 +/- 0.16 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:34:10.65 +25:14:22.7: 14.97 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.12
Forced photometry reference-image weighted average: 15.04 +/- 0.13
Forced photometry filter REJECTED candidate at 23:34:01.66 +23:04:53.8: ref_mag=14.99 +/- 0.12 new_mean_mag=14.9015 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:34:10.65 +25:14:22.7: ref_mag=15.04 +/- 0.13 new_mean_mag=14.8137 delta=0.23 (need > 0.90)
Adding exclusion_list_local.txt__out54834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54945.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 54776_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 54776_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 54779_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 54779_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 54781_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 54781_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 54783_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 54783_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 54784_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 54784_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 54785_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 54785_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 54787_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 54787_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 54793_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 54793_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 54795_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 54795_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 54809_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 54809_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 54811_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 54811_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 54813_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 54813_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 54818_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 54818_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 54825_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 54825_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
**** FOUND 00:01:34.37 +22:43:26.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 54834_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
Preparing report for the candidate 54834_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
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Considering the candidate 54945_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
Preparing report for the candidate 54945_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
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Considering the candidate 55064_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55064_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55069_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55069_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55075_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55075_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55084_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55084_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55090_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55090_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55093_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55093_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55106_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55106_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55108_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55108_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55113_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55113_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55123_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55123_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55124_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55124_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55125_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55125_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55132_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55132_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55141_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55141_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55144_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55144_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55147_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55147_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55158_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55158_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55170_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55170_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55176_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55176_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55177_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55177_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55178_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55178_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55184_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55184_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55185_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55185_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55187_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55187_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55191_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55191_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks
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Considering the candidate 55205_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381
The candidate 55205_fd_Peg-04-Q2b1x1_2026-08-17_03-21-21_20.00sec_-0.00C_LIGHT_0381 did not pass the final checks