This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa
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 12.3703 2461264.8703 12.22 00:04:28.95 +22:11:08.2
108.82205 -39.39618 galactic Peg Second-epoch detections are separated by 0.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.71 Niobe -1 -0 1 12.3 0 0
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:04:28.95 +22:11:08.2: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:04:28.95 +22:11:08.2: 15.93 +/- 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,2461264.8703,12.22,0.05,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 20260812.3703 12.22CV 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 12.3703 2461264.8703 12.38 00:10:07.35 +23:44:01.8
110.88156 -38.16925 galactic Peg Second-epoch detections are separated by 0.3" and 5.2 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 12.6 -0 0
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:10:07.35 +23:44:01.8: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:10:07.35 +23:44:01.8: 16.04 +/- 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,2461264.8703,12.38,0.05,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 20260812.3703 12.38CV 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 12.3703 2461264.8703 14.03 00:06:36.69 +18:21:45.5
108.26783 -43.22909 galactic Peg Second-epoch detections are separated by 1.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.665 Sabine -1 -1 1 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 00:06:36.69 +18:21:45.5: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:06:36.69 +18:21:45.5: 16.02 +/- 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,2461264.8703,14.03,0.05,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 20260812.3703 14.03CV 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
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
target,2461264.8703,14.56,0.05,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
target 20260812.3703 14.56CV 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 12.3703 2461264.8703 14.66 23:38:51.12 +21:07:13.6
101.09159 -38.65336 galactic Peg Second-epoch detections are separated by 0.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.879 Ricarda -1 -1 1 14.4 -0 0
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:38:51.12 +21:07:13.6: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:38:51.12 +21:07:13.6: 15.94 +/- 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,2461264.8703,14.66,0.05,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 20260812.3703 14.66CV 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: 2461264.87060606 12.08.2026 08:53:30.364 /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
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): 7143
Objects passed selection criteria: 7142
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: 6946.25
Average stars matched: 6646.75 (95.6883 %)
Memory usage VmPeak: 234760 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 6 15:05:04 CDT 2026
VaST build number 1.0rc89-190-gdf2934b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Aug 12 04:53:38 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: 2461264.87060606 12.08.2026 08:53:30.364 /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 79
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: 29 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): 43613
Objects passed selection criteria: 43473
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: 42309.2
Average stars matched: 40230 (95.0856 %)
Memory usage VmPeak: 265716 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 6 15:05:04 CDT 2026
VaST build number 1.0rc89-190-gdf2934b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Aug 12 04:55:00 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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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: 2461264.86989549
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
Saving 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'
wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits exists and is non-empty
Saving 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'
wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits exists and is non-empty
Saving wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits to local_wcs_cache/
'wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits' -> 'local_wcs_cache/wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits'
wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits exists and is non-empty
Saving wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits to local_wcs_cache/
'wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits' -> 'local_wcs_cache/wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits'
###################################
# 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_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits (1st new image)
verification OK: wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.563 +22:00:05.72 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 00:00:00.563 +22:00:05.72
Angular distance between the image centers 0.0021 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits (2nd new image)
verification OK: wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:58.684 +21:59:49.09 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 23:59:58.684 +21:59:49.09
Angular distance between the image centers 0.0066 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 00:00:00.563 +22:00:05.72
Second-epoch second image center 23:59:58.684 +21:59:49.09
Angular distance between the image centers 0.00860 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.I4DqKJD4v9
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.RzAATffHNU
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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits &> /tmp/tmp.J9JpbhYnN9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits &> /tmp/tmp.9cvIpBNYZd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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 2 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_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
2.2 pix fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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
15.2 mag. fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
15.2 mag. fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
All-image limiting magnitude estimate: 15.2 (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
############ /tmp/tmp.I4DqKJD4v9 (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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/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.RzAATffHNU (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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/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.J9JpbhYnN9 (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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
Checking if the catalog wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.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_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
WCS catalog name: wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.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=559, bad_region=2066, passed=9130
Got 9130 stars (including 6611 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits.wcscat
util/solve_plate_with_UCAC5 got 9130 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 351.2588 through 0 to 8.7356, gap 8.7356 to 351.2588
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: 4901 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 7492 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 351.2581 through 0 to 8.7358, gap 8.7358 to 351.2581
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 4913 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(), 7492 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 7492 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4904 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=4904 robust_rms=6.642 arcsec worst_quadrant_rms=9.760 arcsec
SIP_REFIT: SIP order 3 trial: matched=4904 robust_rms=0.447 arcsec worst_quadrant_rms=0.558 arcsec
SIP_REFIT: SIP order 5 trial: matched=4904 robust_rms=0.337 arcsec worst_quadrant_rms=0.367 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4904 robust_rms_before=0.889 arcsec robust_rms_before_corrected=0.351 arcsec robust_rms_after=0.337 arcsec worst_quadrant_rms_before=0.382 worst_quadrant_rms_after=0.367
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.382 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits N_match=4904 sigma_overall_arcsec=0.371 sigma_q1_arcsec=0.326 sigma_q2_arcsec=0.381 sigma_q3_arcsec=0.404 sigma_q4_arcsec=0.358 n_q1=1554 n_q2=836 n_q3=1623 n_q4=891 worst_quadrant_to_overall_ratio=1.087
The image catalog is written to wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits -region wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.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.9cvIpBNYZd (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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
Checking if the catalog wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
WCS catalog name: wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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=544, bad_region=2088, passed=9163
Got 9163 stars (including 6635 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits.wcscat
util/solve_plate_with_UCAC5 got 9163 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 351.2317 through 0 to 8.7169, gap 8.7169 to 351.2317
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 4913 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 7499 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 351.2305 through 0 to 8.7170, gap 8.7170 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 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(), 7499 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 7499 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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=6.673 arcsec worst_quadrant_rms=9.559 arcsec
SIP_REFIT: SIP order 3 trial: matched=4907 robust_rms=0.434 arcsec worst_quadrant_rms=0.534 arcsec
SIP_REFIT: SIP order 5 trial: matched=4907 robust_rms=0.329 arcsec worst_quadrant_rms=0.358 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4907 robust_rms_before=0.903 arcsec robust_rms_before_corrected=0.341 arcsec robust_rms_after=0.329 arcsec worst_quadrant_rms_before=0.365 worst_quadrant_rms_after=0.358
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.365 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits N_match=4907 sigma_overall_arcsec=0.364 sigma_q1_arcsec=0.330 sigma_q2_arcsec=0.373 sigma_q3_arcsec=0.387 sigma_q4_arcsec=0.351 n_q1=1547 n_q2=846 n_q3=1628 n_q4=886 worst_quadrant_to_overall_ratio=1.064
The image catalog is written to wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits -region wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-04-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_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits sigma_overall=0.371 worst_q_ratio=1.087
new2=fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits sigma_overall=0.364 worst_q_ratio=1.064
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_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356_astrometric_residuals.png (4904 matched stars from wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357_astrometric_residuals.png (4907 matched stars from wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits'
Saving fully-calibrated image wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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 23:54:54.04 +26:03:43.3: 11.78 +/- 0.01 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:04:28.95 +22:11:08.2: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:54:54.04 +26:03:43.3: 11.76 +/- 0.01 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:04:28.95 +22:11:08.2: 15.93 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Forced photometry filter REJECTED candidate at 23:54:54.04 +26:03:43.3: ref_mag=11.77 +/- 0.01 new_mean_mag=11.9698 delta=-0.20 (need > 0.90)
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
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Considering the candidate 20794_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 20794_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20796_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
Preparing report for the candidate 20796_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
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 ####
00:04:28.95 +22:11:08.2
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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Peg-04-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_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits exists and is non-empty
wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits (1st new image)
verification OK: wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.563 +22:00:05.72 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 00:00:00.563 +22:00:05.72
Angular distance between the image centers 0.0021 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits (2nd new image)
verification OK: wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:58.684 +21:59:49.09 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 23:59:58.684 +21:59:49.09
Angular distance between the image centers 0.0066 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 00:00:00.563 +22:00:05.72
Second-epoch second image center 23:59:58.684 +21:59:49.09
Angular distance between the image centers 0.00860 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.ajnEbduBto
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.fGR2QBjSxP
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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits &> /tmp/tmp.qZ4IiIzx1s
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits &> /tmp/tmp.k7o409fSL0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
2.1 pix fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
15.4 mag. fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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.ajnEbduBto (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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/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 - not rewriting the WCS of whatever it points to, keeping the original solution
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.fGR2QBjSxP (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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/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 - not rewriting the WCS of whatever it points to, keeping the original solution
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.qZ4IiIzx1s (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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
Checking if the catalog wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.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_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
WCS catalog name: wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.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=28, blended=2597, bad_region=9075, passed=52095
Got 52095 stars (including 40881 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits.wcscat
util/solve_plate_with_UCAC5 got 52095 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 351.2302 through 0 to 8.7360, gap 8.7360 to 351.2302
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 4913 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 45288 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 351.2293 through 0 to 8.7361, gap 8.7361 to 351.2293
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 4913 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(), 45288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 45288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits N_match=4906 sigma_overall_arcsec=0.365 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.372 sigma_q3_arcsec=0.410 sigma_q4_arcsec=0.346 n_q1=1573 n_q2=844 n_q3=1611 n_q4=878 worst_quadrant_to_overall_ratio=1.124
The image catalog is written to wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits -region wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.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.k7o409fSL0 (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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
WCS_IMAGE_NAME=wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
WCS-calibrated image found: wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
Checking if the catalog wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits.wcscat corresponding to the image wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits
WCS catalog name: wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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=18, blended=2612, bad_region=9075, passed=52099
Got 52099 stars (including 40835 good ones) from the SExtractor catalog wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits.wcscat
util/solve_plate_with_UCAC5 got 52099 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 351.2289 through 0 to 8.7349, gap 8.7349 to 351.2289
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 4910 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4903 matched stars entering correct_measured_positions(), 45262 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 351.2280 through 0 to 8.7351, gap 8.7351 to 351.2280
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
Accuracy estimation diagnostic: 4903 matched stars entering correct_measured_positions(), 45262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4903 matched stars entering correct_measured_positions(), 45262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits N_match=4903 sigma_overall_arcsec=0.355 sigma_q1_arcsec=0.329 sigma_q2_arcsec=0.366 sigma_q3_arcsec=0.383 sigma_q4_arcsec=0.333 n_q1=1592 n_q2=840 n_q3=1598 n_q4=873 worst_quadrant_to_overall_ratio=1.079
The image catalog is written to wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits -region wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-52-28_20.00sec_-0.00C_LIGHT_0356.fits
Saving fully-calibrated image wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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_2026-08-12_CI_Peg-04-Q2b1x1_044928_TTUQ2b1x1_1862259_FuYF0Txa/wcs_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357.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 23:30:04.63 +23:55:28.0: 14.93 +/- 0.20 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:39:24.25 +24:39:49.6: 14.29 +/- 0.09 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:46:54.22 +22:21:24.6: 14.33 +/- 0.09 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:35:57.77 +22:11:02.4: 14.55 +/- 0.12 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:54:18.46 +18:42:08.7: 14.63 +/- 0.11 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:51:06.58 +23:32:15.6: 14.76 +/- 0.12 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:44:20.06 +19:45:41.9: 14.88 +/- 0.15 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:57:46.98 +19:46:02.4: 14.30 +/- 0.08 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 +21:19:50.7: 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 00:10:07.35 +23:44:01.8: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:35:57.77 +22:11:02.4: 14.72 +/- 0.12 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:39:24.25 +24:39:49.6: 14.57 +/- 0.10 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:30:04.63 +23:55:28.0: 14.51 +/- 0.11 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:54:18.46 +18:42:08.7: 14.66 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.09
Forced photometry reference-image weighted average: 14.42 +/- 0.07
Forced photometry filter REJECTED candidate at 23:35:57.77 +22:11:02.4: ref_mag=14.63 +/- 0.09 new_mean_mag=14.5791 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 14.62 +/- 0.10
Forced photometry filter REJECTED candidate at 23:39:24.25 +24:39:49.6: ref_mag=14.42 +/- 0.07 new_mean_mag=14.7866 delta=-0.37 (need > 0.90)
Forced photometry reference-image weighted average: 14.64 +/- 0.08
Forced photometry filter REJECTED candidate at 23:30:04.63 +23:55:28.0: ref_mag=14.62 +/- 0.10 new_mean_mag=14.7226 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:54:18.46 +18:42:08.7: ref_mag=14.64 +/- 0.08 new_mean_mag=14.6854 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:46:54.22 +22:21:24.6: 14.32 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.06
Forced photometry filter REJECTED candidate at 23:46:54.22 +22:21:24.6: ref_mag=14.32 +/- 0.06 new_mean_mag=14.7183 delta=-0.40 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:15:47.06 +21:19:50.7: 10.40 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.38 +/- 0.00
Forced photometry filter REJECTED candidate at 00:15:47.06 +21:19:50.7: ref_mag=10.38 +/- 0.00 new_mean_mag=10.3951 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:57:46.98 +19:46:02.4: 14.23 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.05
Forced photometry filter REJECTED candidate at 23:57:46.98 +19:46:02.4: ref_mag=14.26 +/- 0.05 new_mean_mag=14.4921 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 23:51:06.58 +23:32:15.6: 14.97 +/- 0.13 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:44:20.06 +19:45:41.9: 14.80 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.10
Forced photometry reference-image weighted average: 14.86 +/- 0.09
Forced photometry filter REJECTED candidate at 23:44:20.06 +19:45:41.9: ref_mag=14.83 +/- 0.10 new_mean_mag=14.7806 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:51:06.58 +23:32:15.6: ref_mag=14.86 +/- 0.09 new_mean_mag=14.7507 delta=0.11 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:10:07.35 +23:44:01.8: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:06:36.69 +18:21:45.5: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:34:41.03 +19:11:42.7: 14.87 +/- 0.18 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:42:45.52 +24:50:29.2: 14.77 +/- 0.14 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:02:07.97 +23:25:30.6: 13.97 +/- 0.06 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:19:03.26 +25:07:33.9: 15.12 +/- 0.18 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:33:27.77 +19:26:48.5: 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 23:42:00.59 +20:10:21.1: 14.50 +/- 0.11 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:06:36.69 +18:21:45.5: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:38:51.12 +21:07:13.6: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:02:07.97 +23:25:30.6: 14.04 +/- 0.05 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:34:41.03 +19:11:42.7: 14.87 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.12
Forced photometry reference-image weighted average: 14.00 +/- 0.04
Forced photometry filter REJECTED candidate at 23:34:41.03 +19:11:42.7: ref_mag=14.87 +/- 0.12 new_mean_mag=14.5775 delta=0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:02:07.97 +23:25:30.6: ref_mag=14.00 +/- 0.04 new_mean_mag=14.2501 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:19:03.26 +25:07:33.9: 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 23:42:45.52 +24:50:29.2: 14.75 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.10
Forced photometry reference-image weighted average: 14.76 +/- 0.09
Forced photometry filter REJECTED candidate at 00:19:03.26 +25:07:33.9: ref_mag=14.95 +/- 0.10 new_mean_mag=14.6550 delta=0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:42:45.52 +24:50:29.2: ref_mag=14.76 +/- 0.09 new_mean_mag=14.5184 delta=0.24 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:33:27.77 +19:26:48.5: 15.07 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.07 +/- 0.13
Forced photometry filter REJECTED candidate at 23:33:27.77 +19:26:48.5: ref_mag=15.07 +/- 0.13 new_mean_mag=14.6194 delta=0.45 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:42:00.59 +20:10:21.1: 14.39 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.07
Forced photometry filter REJECTED candidate at 23:42:00.59 +20:10:21.1: ref_mag=14.44 +/- 0.07 new_mean_mag=14.6492 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:38:51.12 +21:07:13.6: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:30:54.71 +24:19:36.4: 14.99 +/- 0.20 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:32:18.80 +23:49:43.0: 14.48 +/- 0.14 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:33:49.63 +21:06:51.7: 15.10 +/- 0.19 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:43:36.38 +22:14:13.4: 14.73 +/- 0.12 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:41:06.41 +25:10:07.1: 14.82 +/- 0.14 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:34:01.43 +23:04:53.1: 14.98 +/- 0.18 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:32:18.80 +23:49:43.0: 14.57 +/- 0.13 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:43:36.38 +22:14:13.4: 14.75 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.10
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:34:01.43 +23:04:53.1: 15.00 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.08
Forced photometry filter REJECTED candidate at 23:32:18.80 +23:49:43.0: ref_mag=14.52 +/- 0.10 new_mean_mag=14.6949 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 23:41:06.41 +25:10:07.1: 14.99 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 23:43:36.38 +22:14:13.4: ref_mag=14.74 +/- 0.08 new_mean_mag=14.7131 delta=0.03 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:33:49.63 +21:06:51.7: 14.72 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.12
Forced photometry filter REJECTED candidate at 23:34:01.43 +23:04:53.1: ref_mag=14.99 +/- 0.12 new_mean_mag=14.8392 delta=0.15 (need > 0.90)
Forced photometry reference-image weighted average: 14.90 +/- 0.10
Forced photometry filter REJECTED candidate at 23:41:06.41 +25:10:07.1: ref_mag=14.90 +/- 0.10 new_mean_mag=14.7920 delta=0.11 (need > 0.90)
Forced photometry reference-image weighted average: 14.83 +/- 0.11
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:30:54.71 +24:19:36.4: 14.80 +/- 0.15 detection
Forced photometry filter REJECTED candidate at 23:33:49.63 +21:06:51.7: ref_mag=14.83 +/- 0.11 new_mean_mag=14.7289 delta=0.10 (need > 0.90)
Forced photometry reference-image weighted average: 14.87 +/- 0.12
Forced photometry filter REJECTED candidate at 23:30:54.71 +24:19:36.4: ref_mag=14.87 +/- 0.12 new_mean_mag=14.6766 delta=0.19 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:32:31.66 +22:38:35.4: 15.29 +/- 0.25 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:09:36.82 +19:07:57.6: 14.50 +/- 0.10 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:33:42.25 +20:15:25.0: 14.84 +/- 0.16 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:37:53.02 +18:27:00.4: 14.76 +/- 0.18 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:14:50.90 +20:15:56.2: 14.95 +/- 0.15 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:32:29.84 +18:01:39.2: 15.63 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:32:31.66 +22:38:35.4: 15.02 +/- 0.17 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:09:36.82 +19:07:57.6: 14.87 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.14
Forced photometry filter REJECTED candidate at 23:32:31.66 +22:38:35.4: ref_mag=15.10 +/- 0.14 new_mean_mag=14.7471 delta=0.36 (need > 0.90)
Forced photometry reference-image weighted average: 14.62 +/- 0.08
Forced photometry filter REJECTED candidate at 00:09:36.82 +19:07:57.6: ref_mag=14.62 +/- 0.08 new_mean_mag=14.6731 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:37:53.02 +18:27:00.4: 15.11 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.13
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:14:50.90 +20:15:56.2: 15.02 +/- 0.15 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:33:42.25 +20:15:25.0: 14.85 +/- 0.15 detection
Forced photometry filter REJECTED candidate at 23:37:53.02 +18:27:00.4: ref_mag=14.91 +/- 0.13 new_mean_mag=14.7878 delta=0.12 (need > 0.90)
Forced photometry reference-image weighted average: 14.85 +/- 0.11
Forced photometry reference-image weighted average: 14.98 +/- 0.11
Forced photometry filter REJECTED candidate at 23:33:42.25 +20:15:25.0: ref_mag=14.85 +/- 0.11 new_mean_mag=14.9080 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:14:50.90 +20:15:56.2: ref_mag=14.98 +/- 0.11 new_mean_mag=14.8163 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 23:32:29.84 +18:01:39.2: 15.06 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.06 +/- 0.20
Forced photometry filter REJECTED candidate at 23:32:29.84 +18:01:39.2: ref_mag=15.06 +/- 0.20 new_mean_mag=14.8380 delta=0.22 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 00:15:53.53 +24:52:54.0: 14.62 +/- 0.11 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:58:04.73 +24:00:24.1: 14.90 +/- 0.15 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:38:27.15 +24:53:56.9: 14.85 +/- 0.15 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:38:09.30 +24:15:37.5: 15.20 +/- 0.22 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:40:16.80 +17:45:44.8: 14.95 +/- 0.18 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 00:15:53.53 +24:52:54.0: 14.63 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.08
Forced photometry filter REJECTED candidate at 00:15:53.53 +24:52:54.0: ref_mag=14.63 +/- 0.08 new_mean_mag=14.7920 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 23:30:57.53 +23:21:43.9: 14.99 +/- 0.19 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:58:04.73 +24:00:24.1: 15.05 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.11
Forced photometry filter REJECTED candidate at 23:58:04.73 +24:00:24.1: ref_mag=14.97 +/- 0.11 new_mean_mag=14.8797 delta=0.09 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:38:27.15 +24:53:56.9: 15.03 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.11
Forced photometry filter REJECTED candidate at 23:38:27.15 +24:53:56.9: ref_mag=14.93 +/- 0.11 new_mean_mag=14.7533 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 23:38:09.30 +24:15:37.5: 15.55 +/- 0.27 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:40:16.80 +17:45:44.8: 15.20 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.17
Forced photometry reference-image weighted average: 15.06 +/- 0.14
Forced photometry filter REJECTED candidate at 23:40:16.80 +17:45:44.8: ref_mag=15.06 +/- 0.14 new_mean_mag=14.8817 delta=0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:38:09.30 +24:15:37.5: ref_mag=15.33 +/- 0.17 new_mean_mag=14.8069 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 23:30:57.53 +23:21:43.9: 14.89 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.12
Forced photometry filter REJECTED candidate at 23:30:57.53 +23:21:43.9: ref_mag=14.93 +/- 0.12 new_mean_mag=14.8428 delta=0.09 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:31:54.84 +20:14:27.8: 15.31 +/- 0.26 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:39:51.05 +24:30:41.1: 15.28 +/- 0.23 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-17_05-23-21_20.00sec_4.90C_LIGHT_0302.fits at 23:33:19.76 +25:53:11.9: 14.89 +/- 0.18 detection
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:31:54.84 +20:14:27.8: 15.36 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.34 +/- 0.18
Forced photometry filter REJECTED candidate at 23:31:54.84 +20:14:27.8: ref_mag=15.34 +/- 0.18 new_mean_mag=14.9367 delta=0.40 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:39:51.05 +24:30:41.1: 15.28 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.28 +/- 0.15
Forced photometry filter REJECTED candidate at 23:39:51.05 +24:30:41.1: ref_mag=15.28 +/- 0.15 new_mean_mag=14.9181 delta=0.36 (need > 0.90)
Forced photometry on wcs_Peg-04-Q2b1x1_2026-07-21_04-02-11_20.00sec_5.00C_LIGHT_0930.fits at 23:33:19.76 +25:53:11.9: 15.34 +/- 0.25 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.15
Forced photometry filter REJECTED candidate at 23:33:19.76 +25:53:11.9: ref_mag=15.05 +/- 0.15 new_mean_mag=14.9470 delta=0.10 (need > 0.90)
Adding exclusion_list_local.txt__out54829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54949.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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: 4s
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Considering the candidate 54781_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54781_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54783_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54783_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54785_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54785_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54786_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54786_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54790_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54790_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54793_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54793_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54797_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54797_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54798_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54798_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54820_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54820_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54827_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54827_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
**** FOUND 00:04:28.95 +22:11:08.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 54829_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
Preparing report for the candidate 54829_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
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Considering the candidate 54884_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
Preparing report for the candidate 54884_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
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Considering the candidate 54901_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54901_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54916_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54916_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54930_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54930_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54936_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54936_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54940_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
Preparing report for the candidate 54940_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
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Considering the candidate 54948_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54948_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54949_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
Preparing report for the candidate 54949_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
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Considering the candidate 54953_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54953_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54954_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54954_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54960_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54960_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54965_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54965_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54968_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54968_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54979_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54979_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54985_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54985_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54990_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54990_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54992_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54992_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 54994_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 54994_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 55003_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 55003_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 55008_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 55008_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 55013_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 55013_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 55014_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 55014_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 55015_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 55015_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 55018_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 55018_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 55021_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 55021_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 55022_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 55022_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 55030_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 55030_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 55031_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 55031_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 55033_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 55033_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 55038_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 55038_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
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Considering the candidate 52763_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357
The candidate 52763_fd_Peg-04-Q2b1x1_2026-08-12_03-53-30_20.00sec_0.00C_LIGHT_0357 did not pass the final checks
