This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF
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 05 13.4239 2461173.9239 8.55 00:06:29.23 +27:05:25.7
110.74675 -34.71544 galactic Peg Second-epoch detections are separated by 0.3" and 3.4 pix
The object was found in VSX 1" TT Peg
Type: SRA
# Max. Min./Amp. JD0 Period
9.300 V 11.200 V 2437178.00000 154.000000000000 M6e
The object was not found in astcheck.
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:06:29.23 +27:05:25.7: 9.75 +/- 0.00 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:06:29.23 +27:05:25.7: 15.85 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 9.75 +/- 0.00
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
TT Peg,2461173.9239,8.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TT Peg 20260513.4239 8.55CV 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 05 13.4239 2461173.9239 8.29 00:22:23.13 +26:59:46.4
114.98559 -35.42686 galactic And Second-epoch detections are separated by 0.3" and 3.5 pix
The object was found in VSX 1" T And
Type: M
# Max. Min./Amp. JD0 Period
7.700 V 14.500 V 2450854.00000 281.000000000000 M4e-M7.5e
The object was not found in astcheck.
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:22:23.13 +26:59:46.4: 10.67 +/- 0.00 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:22:23.13 +26:59:46.4: 15.61 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 10.67 +/- 0.00
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!
TCP 2026 05 13.4239* 00 22 23.13 +26 59 46.4 8.3 U And 9 0
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
T And,2461173.9239,8.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
T And 20260513.4239 8.29CV 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 05 13.4239 2461173.9239 10.63 00:14:10.90 +29:01:20.5
113.20083 -33.14444 galactic And Second-epoch detections are separated by 0.4" and 3.4 pix
The object was found in VSX 0" UW And
Type: M
# Max. Min./Amp. JD0 Period
9.400 V < 15.000 V 2454024.00000 237.000000000000 M5
The object was not found in astcheck.
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:14:10.90 +29:01:20.5: 11.62 +/- 0.01 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:14:10.90 +29:01:20.5: 15.84 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.62 +/- 0.01
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!
TCP 2026 05 13.4239* 00 14 10.90 +29 01 20.5 10.6 U And 9 0
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
UW And,2461173.9239,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
UW And 20260513.4239 10.63CV 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 05 13.4239 2461173.9239 10.64 00:27:14.15 +30:53:48.0
116.83018 -31.68818 galactic And Second-epoch detections are separated by 0.2" and 3.4 pix
The object was found in VSX 1" YZ And
Type: M
# Max. Min./Amp. JD0 Period
9.700 V 15.900 V 2454092.00000 207.000000000000 M5e
The object was not found in astcheck.
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:27:14.15 +30:53:48.0: 13.44 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:27:14.15 +30:53:48.0: 14.28 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
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!
TCP 2026 05 13.4239* 00 27 14.15 +30 53 48.0 10.6 U And 9 0
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
YZ And,2461173.9239,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
YZ And 20260513.4239 10.64CV 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 05 13.4239 2461173.9239 10.34 23:51:44.08 +29:45:43.3
107.75495 -31.34412 galactic Peg Second-epoch detections are separated by 0.3" and 3.3 pix
The object was found in VSX 0" DU Peg
Type: M
# Max. Min./Amp. JD0 Period
11.000 pg < 15.000 pg 2429253.00000 161.300000000000 M5e
The object was not found in astcheck.
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:51:44.08 +29:45:43.3: 13.25 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:51:44.08 +29:45:43.3: 16.07 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.25 +/- 0.03
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
DU Peg,2461173.9239,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DU Peg 20260513.4239 10.34CV 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: 2461032.65010065 23.12.2025 03:35:58.696 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
First image: 2461032.65010065 23.12.2025 03:35:58.696 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Last image: 2461173.92414369 13.05.2026 10:10:36.015 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.53
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: 7 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 11456
Objects passed selection criteria: 11418
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 9820.75
Average stars matched: 9692.75 (98.6966 %)
Memory usage VmPeak: 117012 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 10 15:05:05 CDT 2026
VaST build number 1.0rc89-44-gd532a530
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed May 13 06:32:08 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: 2461032.65010065 23.12.2025 03:35:58.696 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
First image: 2461032.65010065 23.12.2025 03:35:58.696 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Last image: 2461173.92414369 13.05.2026 10:10:36.015 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 75
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
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: 34 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 70638
Objects passed selection criteria: 70503
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 62463.8
Average stars matched: 61158 (97.9096 %)
Memory usage VmPeak: 1858592 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 10 15:05:05 CDT 2026
VaST build number 1.0rc89-44-gd532a530
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed May 13 06:35:27 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
SExtractor catalog cache: saved Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat to cache
SExtractor catalog cache: saved Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.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-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.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: 2461173.92370322
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
Entering WCS image calibration mode.
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Entering WCS image calibration mode.
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
WCS_IMAGE_NAME=wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits was not set. Trying to guess...
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
The guess is 605 arcmin.
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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
WCS_IMAGE_NAME=wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits was not set. Trying to guess...
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits .... Determining astrometry method...
The guess is 605 arcmin.
It's a known telescope with plate solutions that are supposed to be good.
Using the local copy of Astrometry.net software...
Choosing aperture...
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits has a WCS header - will blindly trust it is good...
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits' -> 'wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits was not set. Trying to guess...
The guess is 568 arcmin.
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits .... Determining astrometry method...
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits has a WCS header - will blindly trust it is good...
WCS-calibrated image found: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Checking if the catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits was not found.
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits' -> 'wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
WCS_IMAGE_NAME=wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits was not set. Trying to guess...
The guess is 572 arcmin.
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
WCS-calibrated image found: wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Checking if the catalog wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits alredy exist and is non-empty...
Catalog wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits was not found.
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/lib/make_outxyls_for_astrometric_calibration found 7360 high-SNR stars for plate solving
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
verification OK: wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/lib/make_outxyls_for_astrometric_calibration found 7383 high-SNR stars for plate solving
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
Generating wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat from image00002.cat
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Using the local copy of Astrometry.net code
Generating wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat from image00001.cat
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out2590949.xyls"...
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out2590943.xyls"...
Catalog wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits created.
verification OK: wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits created.
verification OK: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Image size: 931.4'x628.9' 15.5(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.91"/pix along the Y axis
Image center: 00:00:08.789 +30:01:35.04 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:59.947 +29:59:55.87 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 11750 stars ###
'wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/correct_sextractor_wcs_catalog_usingxy2sky2591959.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
### Converted positions of 12651 stars ###
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
'wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
Reading file "./out2590949.axy"...
Reading file "./out2590943.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4114.fits, field objects 1-10).
Field 1 did not solve (index index-4113.fits, field objects 1-10).
Field 1 did not solve (index index-4112.fits, field objects 1-10).
Field 1 did not solve (index index-4111.fits, field objects 1-10).
Field 1 did not solve (index index-4110.fits, field objects 1-10).
Field 1 did not solve (index index-4109.fits, field objects 1-10).
Field 1 did not solve (index index-4108.fits, field objects 1-10).
Field 1 did not solve (index index-4119.fits, field objects 11-20).
Field 1 did not solve (index index-4118.fits, field objects 11-20).
Field 1 did not solve (index index-4117.fits, field objects 11-20).
log-odds ratio 33.8012 (4.78252e+14), 7 match, 0 conflict, 6 distractors, 28 index.
RA,Dec = (0.00426993,30.0063), pixel scale 5.96884 arcsec/pix.
Hit/miss: Hit/miss: ++------+++++(best)----------+---------+--------------------+---------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2590949.solved to indicate this.
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
Field 1 did not solve (index index-4116.fits, field objects 1-10).
Field 1 did not solve (index index-4115.fits, field objects 1-10).
Field 1 did not solve (index index-4114.fits, field objects 1-10).
Field 1 did not solve (index index-4113.fits, field objects 1-10).
Field 1 did not solve (index index-4112.fits, field objects 1-10).
Field 1 did not solve (index index-4111.fits, field objects 1-10).
Field 1 did not solve (index index-4110.fits, field objects 1-10).
Field 1 did not solve (index index-4109.fits, field objects 1-10).
Field 1 did not solve (index index-4108.fits, field objects 1-10).
Field 1 did not solve (index index-4119.fits, field objects 11-20).
Field 1 did not solve (index index-4118.fits, field objects 11-20).
Field 1 did not solve (index index-4117.fits, field objects 11-20).
Field 1 did not solve (index index-4116.fits, field objects 11-20).
log-odds ratio 54.7154 (5.78886e+23), 16 match, 0 conflict, 40 distractors, 46 index.
RA,Dec = (0.00585325,29.9987), pixel scale 5.97901 arcsec/pix.
Hit/miss: Hit/miss: -+--+--+--+--+-+-----++--+--+--+-----+-----------+-++--+(best)-----------------------------+--------------
Field 1: solved with index index-4115.fits.
Field 1 solved: writing to file ./out2590943.solved to indicate this.
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/correct_sextractor_wcs_catalog_usingxy2sky2591895.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Field: out2590949.xyls
Field center: (RA,Dec) = (0.005649, 30.008913) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:01.356, +30:00:32.085).
Field size: 15.809 x 10.5794 degrees
Field rotation angle: up is 3.40719 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits' -> 'fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits'
Field: out2590943.xyls
Field center: (RA,Dec) = (0.004479, 30.002301) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:01.075, +30:00:08.283).
Field size: 15.8077 x 10.5772 degrees
Field rotation angle: up is 3.41139 degrees E of N
Field parity: neg
Inserting WCS header... WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 13 06:32 fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
-rw-r--r-- 1 apache apache 12K May 13 06:32 out2590949.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits for reading... done!
Creating new image file (wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits)... done!
'/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits' -> 'fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits'
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 13 06:32 fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
-rw-r--r-- 1 apache apache 12K May 13 06:32 out2590943.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits for reading... done!
Creating new image file (wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits)... done!
done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits (fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out2590949.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2590949.axy"...
Only searching for solutions within 15.765 degrees of RA,Dec (0.0066625,30.0097)
log-odds ratio 33.8012 (4.78252e+14), 7 match, 0 conflict, 6 distractors, 28 index.
RA,Dec = (0.00426993,30.0063), pixel scale 5.96884 arcsec/pix.
Hit/miss: Hit/miss: ++------+++++(best)----------+---------+--------------------+---------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2590949.solved to indicate this.
Field: out2590949.xyls
Field center: (RA,Dec) = (0.004114, 30.007026) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:00.987, +30:00:25.295).
Field size: 15.79 x 10.5763 degrees
Field rotation angle: up is 3.41164 degrees E of N
Field parity: neg
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits (fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 13 06:32 fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
-rw-r--r-- 1 apache apache 12K May 13 06:32 out2590949.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits for reading... done!
Creating new image file (wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits)... done!
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
done!
Reading input file 1 of 1: "out2590943.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2590943.axy"...
Only searching for solutions within 15.7483 degrees of RA,Dec (0.00549167,30.0031)
log-odds ratio 33.89 (5.22669e+14), 7 match, 0 conflict, 6 distractors, 28 index.
RA,Dec = (0.00236242,30.001), pixel scale 5.96888 arcsec/pix.
Hit/miss: Hit/miss: ++------+++++(best)----------+---------+------------------------+-----------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2590943.solved to indicate this.
Field: out2590943.xyls
Field center: (RA,Dec) = (0.002166, 30.001693) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:00.520, +30:00:06.096).
Field size: 15.7904 x 10.5763 degrees
Field rotation angle: up is 3.41096 degrees E of N
Field parity: neg
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 13 06:32 fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
-rw-r--r-- 1 apache apache 12K May 13 06:32 out2590943.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits for reading... done!
Creating new image file (wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 38179 sources.
Solving...
Reading file "./wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.axy"...
Verifying WCS using indices with quads of size [63.7534, 955.702] arcmin
Verifying WCS with index 39 of 61 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 40 of 61 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
log-odds ratio 132.893 (5.18488e+57), 27 match, 0 conflict, 370 distractors, 28 index.
RA,Dec = (0.0030982,30.0062), pixel scale 5.98811 arcsec/pix.
Hit/miss: Hit/miss: ---------------------------------+-----+------+--+---------------------+--------+------+----+-+-----
--> log-odds 132.893
Verifying WCS with index 41 of 61 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 319.434 (5.35162e+138), 44 match, 0 conflict, 353 distractors, 46 index.
RA,Dec = (0.0030982,30.0062), pixel scale 5.98811 arcsec/pix.
Hit/miss: Hit/miss: -----------------------------+---+-----+------+--+-----+----------+----+--------+------+---++-+----+
--> log-odds 319.434
Verifying WCS with index 42 of 61 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 799.522 (inf), 90 match, 0 conflict, 487 distractors, 93 index.
RA,Dec = (0.0030982,30.0062), pixel scale 5.98811 arcsec/pix.
Hit/miss: Hit/miss: ----------+---------+------+-+---++-+--+---+--+--+---+-+--+-------+-+--+---+--+-+-++---+---++++-+--+
--> log-odds 799.522
Verifying WCS with index 43 of 61 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 1793.93 (inf), 190 match, 0 conflict, 403 distractors, 196 index.
RA,Dec = (0.0030982,30.0062), pixel scale 5.98811 arcsec/pix.
Hit/miss: Hit/miss: ++-+--++--+++-+++---++-+-+-+-+-+-++++--++++++++--++-++-+-++--+-+-++-++-+++-+-++-++++--++--+++++-+-++
--> log-odds 1793.93
Verifying WCS with index 44 of 61 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 3431.12 (inf), 375 match, 0 conflict, 341 distractors, 384 index.
RA,Dec = (0.0030982,30.0062), pixel scale 5.98811 arcsec/pix.
Hit/miss: Hit/miss: ++++-+++-++++++++++-++-+-+++++++-++++++++++++++-++++++++++++++-+++++++++++++++++++++-++++-++++++++++
--> log-odds 3431.12
Verifying WCS with index 45 of 61 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 6207.33 (inf), 725 match, 0 conflict, 1278 distractors, 741 index.
RA,Dec = (0.0030982,30.0062), pixel scale 5.98811 arcsec/pix.
Hit/miss: Hit/miss: ++++++++++++++++++++++-+++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
--> log-odds 6207.33
Verifying WCS with index 46 of 61 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 11359.2 (inf), 1434 match, 0 conflict, 2066 distractors, 1458 index.
RA,Dec = (0.0030982,30.0062), pixel scale 5.98811 arcsec/pix.
Hit/miss: Hit/miss: ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
--> log-odds 11359.2
Got 7 solutions.
Field: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Field center: (RA,Dec) = (0.004700, 30.006193) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:01.128, +30:00:22.296).
Field size: 15.7873 x 10.5753 degrees
Field rotation angle: up is 3.40647 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.new"...
renamed 'wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.new' -> 'wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits'
Checking if the catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Generating wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat from image00004.cat
Catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits created.
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Image size: 942.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:01.372 +30:00:25.10 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 7558 stars ###
'wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/correct_sextractor_wcs_catalog_usingxy2sky2626939.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
simplexy: found 37948 sources.
Solving...
Reading file "./wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.axy"...
Verifying WCS using indices with quads of size [63.7532, 955.699] arcmin
Verifying WCS with index 39 of 61 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 0
Verifying WCS with index 40 of 61 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
log-odds ratio 127.309 (1.94737e+55), 27 match, 0 conflict, 393 distractors, 28 index.
RA,Dec = (0.00115032,30.0009), pixel scale 5.98809 arcsec/pix.
Hit/miss: Hit/miss: ----------------------------------+---++-------------------------------+-+-----++----++-------------
--> log-odds 127.309
Verifying WCS with index 41 of 61 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 321.546 (4.42258e+139), 44 match, 0 conflict, 376 distractors, 46 index.
RA,Dec = (0.00115032,30.0009), pixel scale 5.98809 arcsec/pix.
Hit/miss: Hit/miss: ---------------------+------------+---++----+---------+---++-----------+-+-----++----++-------------
--> log-odds 321.546
Verifying WCS with index 42 of 61 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 799.436 (inf), 90 match, 0 conflict, 511 distractors, 93 index.
RA,Dec = (0.00115032,30.0009), pixel scale 5.98809 arcsec/pix.
Hit/miss: Hit/miss: ------------+--------+------+-----++--++----++---+-++-++--++------+++--+-+-+---++----++--------+---+
--> log-odds 799.436
Verifying WCS with index 43 of 61 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 1795.16 (inf), 190 match, 0 conflict, 435 distractors, 196 index.
RA,Dec = (0.00115032,30.0009), pixel scale 5.98809 arcsec/pix.
Hit/miss: Hit/miss: ++-+++++-++-++++----++-+----++-+++++-+++-++-++--++++++++--++-+++--++++++-+++---++-++-++----+-------+
--> log-odds 1795.16
Verifying WCS with index 44 of 61 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 3445.39 (inf), 376 match, 0 conflict, 355 distractors, 385 index.
RA,Dec = (0.00115032,30.0009), pixel scale 5.98809 arcsec/pix.
Hit/miss: Hit/miss: ++++++++-+++++++++++++-+-+++++++++++-++++++++++-++++++++++++++++++++++++++++++++++++++++++++++++++-+
--> log-odds 3445.39
Verifying WCS with index 45 of 61 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 6224.58 (inf), 726 match, 0 conflict, 1062 distractors, 742 index.
RA,Dec = (0.00115032,30.0009), pixel scale 5.98809 arcsec/pix.
Hit/miss: Hit/miss: ++++++++++++++++++++++-+++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
--> log-odds 6224.58
Verifying WCS with index 46 of 61 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 11394.1 (inf), 1437 match, 0 conflict, 2535 distractors, 1461 index.
RA,Dec = (0.00115032,30.0009), pixel scale 5.98809 arcsec/pix.
Hit/miss: Hit/miss: ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
--> log-odds 11394.1
Got 7 solutions.
Field: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Field center: (RA,Dec) = (0.002779, 30.000859) deg.
Field center: (RA H:M:S, Dec D:M:S) = (00:00:00.667, +30:00:03.092).
Field size: 15.7875 x 10.5753 degrees
Field rotation angle: up is 3.40659 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.new"...
renamed 'wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.new' -> 'wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits'
Checking if the catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Generating wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat from image00003.cat
Catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits created.
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Image size: 942.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:00.911 +30:00:05.90 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 7554 stars ###
'wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/correct_sextractor_wcs_catalog_usingxy2sky2628671.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits exists and is non-empty
Saving wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits to local_wcs_cache/
'wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits' -> 'local_wcs_cache/wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits'
wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits exists and is non-empty
Saving wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits to local_wcs_cache/
'wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits' -> 'local_wcs_cache/wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits'
wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits exists and is non-empty
Saving wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits to local_wcs_cache/
'wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits' -> 'local_wcs_cache/wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits'
wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits exists and is non-empty
Saving wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits to local_wcs_cache/
'wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits' -> 'local_wcs_cache/wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits (1st reference image)
verification OK: wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:59.947 +29:59:55.87 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits (1st new image)
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Image size: 942.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:00.911 +30:00:05.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:59.947 +29:59:55.87
Second-epoch image center 00:00:00.911 +30:00:05.90
Angular distance between the image centers 0.0045 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits (2nd new image)
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Image size: 942.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:01.372 +30:00:25.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:59.947 +29:59:55.87
Second-epoch image center 00:00:01.372 +30:00:25.10
Angular distance between the image centers 0.0096 deg.
###################################
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits sigma_overall=N/A worst_q_ratio=N/A
ref2=wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits sigma_overall=N/A worst_q_ratio=N/A
new1=wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits sigma_overall=N/A worst_q_ratio=N/A
new2=wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits sigma_overall=N/A worst_q_ratio=N/A
reference average sigma_overall=N/A worst_q_ratio=N/A
warn-on-ratio threshold: 2.0x reference
###################################
INFO: WCS quality sigma_overall_arcsec not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality sigma_overall_arcsec not available for comparison (2nd new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (2nd new image new=N/A ref_avg=N/A)
###################################
# 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 00:00:00.911 +30:00:05.90
Second-epoch second image center 00:00:01.372 +30:00:25.10
Angular distance between the image centers 0.00559 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits &> /tmp/tmp.WCBPmlvGt7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits &> /tmp/tmp.FykXxGNvl2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits &> /tmp/tmp.9uT95Uoxb3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits &> /tmp/tmp.nbglZ8tIof
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.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-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits and wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat
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-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits and wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat
Found non-empty wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits and wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat
The reference image (wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits) and catalog (wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat) found
'wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat' -> 'wcsmag.cat'
Read 12651 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0033 to 359.9985 deg, Dec +24.3232 to +35.3077 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 0.0033 to 359.9985 deg, Dec 24.3232 to 35.3077 deg
Loaded 205042 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): 6498 out of 6940 total matches.
Matched with Tycho-2 6940 out of 12651 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.942650
a=0.000000 b=1.000000 c=22.942650
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 12651 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0033 to 359.9985 deg, Dec +24.3232 to +35.3077 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 0.0033 to 359.9985 deg, Dec 24.3232 to 35.3077 deg
Loaded 205042 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): 6498 out of 6940 total matches.
Matched with Tycho-2 6940 out of 12651 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits:
Forced-photometry filter: calibrated wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits -> calib.txt_param_ref_wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits (aperture=5.9)
Read 11750 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0051 to 359.9954 deg, Dec +24.3957 to +35.2760 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 0.0051 to 359.9954 deg, Dec 24.3957 to 35.2760 deg
Loaded 203220 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): 39 out of 41 total matches.
Matched with Tycho-2 41 out of 11750 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits:
Forced-photometry filter: calibrated wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits -> calib.txt_param_ref_wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
2.0 pix Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
2.3 pix fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
2.3 pix fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
2.0 pix wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
2.0 pix wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Limiting magnitude estimates:
15.4 mag. Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
15.3 mag. Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
14.7 mag. fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
14.7 mag. fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.8 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.WCBPmlvGt7 (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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.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-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits' -> 'wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
WCS_IMAGE_NAME=wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
WCS-calibrated image found: wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Checking if the catalog wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits alredy exist and is non-empty...
Catalog wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
WCS catalog name: wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=969, passed=12651
Got 12651 stars (including 11664 good ones) from the SExtractor catalog wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat
util/solve_plate_with_UCAC5 got 12651 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.5839 through 0 to 9.6538, gap 9.6538 to 350.5839
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 12440 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 350.5834 through 0 to 9.6544, gap 9.6544 to 350.5834
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 12442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 12442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits N_match=972 sigma_overall_arcsec=0.336 sigma_q1_arcsec=0.441 sigma_q2_arcsec=0.336 sigma_q3_arcsec=0.326 sigma_q4_arcsec=0.290 n_q1=217 n_q2=272 n_q3=234 n_q4=249 worst_quadrant_to_overall_ratio=1.313
The image catalog is written to wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits -region wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FykXxGNvl2 (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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.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-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits' -> 'wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
WCS-calibrated image found: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Checking if the catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
WCS catalog name: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=866, passed=11750
Got 11750 stars (including 10862 good ones) from the SExtractor catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat
util/solve_plate_with_UCAC5 got 11750 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.4'
Seting catalog search parameters based on the expected field of view 931.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012936 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010349 (37.3 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 350.9179 through 0 to 9.7115, gap 9.7115 to 350.9179
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 205 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 171 matched stars entering correct_measured_positions(), 136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.07"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 167 matched stars entering correct_measured_positions(), 2040 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.03"
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 350.9134 through 0 to 9.7048, gap 9.7048 to 350.9134
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 250 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 225 matched stars entering correct_measured_positions(), 2065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.88"
Accuracy estimation diagnostic: 223 matched stars entering correct_measured_positions(), 2674 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.92"
Excluding outliers - 223 stars left (next iteration limit 183)
WCS_QUALITY_DIAG: file=Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits N_match=223 sigma_overall_arcsec=11.010 sigma_q1_arcsec=6.652 sigma_q2_arcsec=36.650 sigma_q3_arcsec=20.046 sigma_q4_arcsec=41.539 n_q1=141 n_q2=11 n_q3=64 n_q4=7 worst_quadrant_to_overall_ratio=3.773
The image catalog is written to wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits -region wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.9uT95Uoxb3 (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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
WCS_IMAGE_NAME=wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
WCS-calibrated image found: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Checking if the catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
WCS catalog name: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=475, passed=7554
Got 7554 stars (including 7072 good ones) from the SExtractor catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat
util/solve_plate_with_UCAC5 got 7554 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.8092 through 0 to 9.8179, gap 9.8179 to 350.8092
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 7429 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.8088 through 0 to 9.8185, gap 9.8185 to 350.8088
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 7427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 7427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits N_match=965 sigma_overall_arcsec=0.328 sigma_q1_arcsec=0.328 sigma_q2_arcsec=0.342 sigma_q3_arcsec=0.310 sigma_q4_arcsec=0.332 n_q1=241 n_q2=210 n_q3=284 n_q4=230 worst_quadrant_to_overall_ratio=1.044
The image catalog is written to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits -region wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nbglZ8tIof (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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
WCS_IMAGE_NAME=wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
WCS-calibrated image found: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Checking if the catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
WCS catalog name: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=477, passed=7558
Got 7558 stars (including 7072 good ones) from the SExtractor catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat
util/solve_plate_with_UCAC5 got 7558 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.8092 through 0 to 9.8179, gap 9.8179 to 350.8092
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 7450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 350.8089 through 0 to 9.8185, gap 9.8185 to 350.8089
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 7451 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 7451 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits N_match=963 sigma_overall_arcsec=0.324 sigma_q1_arcsec=0.303 sigma_q2_arcsec=0.339 sigma_q3_arcsec=0.293 sigma_q4_arcsec=0.355 n_q1=243 n_q2=210 n_q3=282 n_q4=228 worst_quadrant_to_overall_ratio=1.096
The image catalog is written to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits -region wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits'
Saving fully-calibrated image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits'
Preparing the HTML report for the field Peg-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:27:14.17 +30:53:48.2: 13.28 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:51:44.09 +29:45:43.6: 13.03 +/- 0.02 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:06:29.23 +27:05:25.7: 9.75 +/- 0.00 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:22:23.13 +26:59:46.4: 10.67 +/- 0.00 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:14:10.90 +29:01:20.5: 11.62 +/- 0.01 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:27:14.17 +30:53:48.2: 13.97 +/- 0.07 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:51:44.09 +29:45:43.6: 16.04 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Forced photometry filter KEPT candidate at 00:27:14.17 +30:53:48.2: ref_mag=13.40 +/- 0.03 new_mean_mag=10.5141 delta=2.89 (need > 0.90)
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 23:51:44.09 +29:45:43.6: ref_mag=13.03 +/- 0.02 new_mean_mag=10.1381 delta=2.89 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:22:23.13 +26:59:46.4: 15.61 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:06:29.23 +27:05:25.7: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:14:10.90 +29:01:20.5: 15.84 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter KEPT candidate at 00:06:29.23 +27:05:25.7: ref_mag=9.75 +/- 0.00 new_mean_mag=8.5511 delta=1.20 (need > 0.90)
Forced photometry reference-image weighted average: 10.67 +/- 0.00
Forced photometry filter KEPT candidate at 00:22:23.13 +26:59:46.4: ref_mag=10.67 +/- 0.00 new_mean_mag=8.2915 delta=2.38 (need > 0.90)
Forced photometry reference-image weighted average: 11.62 +/- 0.01
Forced photometry filter KEPT candidate at 00:14:10.90 +29:01:20.5: ref_mag=11.62 +/- 0.01 new_mean_mag=10.6374 delta=0.99 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out20384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out07627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09835.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: 2s
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Considering the candidate 20384_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 20384_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 23:51:44.09 +29:45:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.13, MAG_FAINT_SEARCH_LIMIT=11.11)GAIADR2_OUTPUT=# 0.430 2867412942399525120 357.93365213699 +29.76200219787 9.5153 7.9433 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20403_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 20403_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 00:27:14.17 +30:53:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.51, MAG_FAINT_SEARCH_LIMIT=11.49)GAIADR2_OUTPUT=# 0.920 2859182101432492800 006.80933939944 +30.89672791884 10.9418 9.5559 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20477_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 20477_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 23:49:33.27 +28:51:38.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 09835_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
Preparing report for the candidate 09835_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
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Considering the candidate 09761_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
Preparing report for the candidate 09761_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03430_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 03430_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 23:36:59.63 +32:42:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07627_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
Preparing report for the candidate 07627_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 9s
Prepared the HTML report for the field Peg-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:14:10.90 +29:01:20.5
00:22:23.13 +26:59:46.4
00:06:29.23 +27:05:25.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
SExtractor catalog cache: saved Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat to cache
SExtractor catalog cache: saved Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.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-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Creating symlink local_wcs_cache/wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.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
Entering WCS image calibration mode.
Entering WCS image calibration mode.
Entering WCS image calibration mode.
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
WCS_IMAGE_NAME=wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits was not set. Trying to guess...
The guess is 605 arcmin.
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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
WCS_IMAGE_NAME=wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits was not set. Trying to guess...
The guess is 605 arcmin.
WCS-calibrated image found: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Checking if the catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits was not found.
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits has a WCS header - will blindly trust it is good...
It's a known telescope with plate solutions that are supposed to be good.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits has a WCS header - will blindly trust it is good...
WCS-calibrated image found: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Checking if the catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits' -> 'wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
WCS_IMAGE_NAME=wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits was not set. Trying to guess...
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits' -> 'wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits was not set. Trying to guess...
The guess is 572 arcmin.
The guess is 568 arcmin.
WCS-calibrated image found: wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Checking if the catalog wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits alredy exist and is non-empty...
Catalog wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits was not found.
WCS-calibrated image found: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Checking if the catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Generating wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat from image00003.cat
Generating wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat from image00004.cat
Generating wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat from image00002.cat
Generating wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat from image00001.cat
Catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits created.
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits created.
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits created.
verification OK: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
verification OK: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Image size: 942.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:00.911 +30:00:05.90 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Image size: 931.4'x628.9' 15.5(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.91"/pix along the Y axis
Image center: 00:00:08.789 +30:01:35.04 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Image size: 942.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:01.372 +30:00:25.10 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Catalog wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits created.
verification OK: wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
verification OK: wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:59.947 +29:59:55.87 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 50097 stars ###
'wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/correct_sextractor_wcs_catalog_usingxy2sky2738006.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
### Converted positions of 50376 stars ###
'wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/correct_sextractor_wcs_catalog_usingxy2sky2738020.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
### Converted positions of 73343 stars ###
'wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/correct_sextractor_wcs_catalog_usingxy2sky2738047.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
### Converted positions of 77944 stars ###
'wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/correct_sextractor_wcs_catalog_usingxy2sky2738281.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits exists and is non-empty
wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits exists and is non-empty
wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits exists and is non-empty
wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits (1st reference image)
verification OK: wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Image size: 941.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:59.947 +29:59:55.87 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits (1st new image)
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Image size: 942.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:00.911 +30:00:05.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:59.947 +29:59:55.87
Second-epoch image center 00:00:00.911 +30:00:05.90
Angular distance between the image centers 0.0045 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits (2nd new image)
verification OK: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Image size: 942.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:01.372 +30:00:25.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:59.947 +29:59:55.87
Second-epoch image center 00:00:01.372 +30:00:25.10
Angular distance between the image centers 0.0096 deg.
###################################
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits sigma_overall=N/A worst_q_ratio=N/A
ref2=wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits sigma_overall=N/A worst_q_ratio=N/A
new1=wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits sigma_overall=N/A worst_q_ratio=N/A
new2=wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits sigma_overall=N/A worst_q_ratio=N/A
reference average sigma_overall=N/A worst_q_ratio=N/A
warn-on-ratio threshold: 2.0x reference
###################################
INFO: WCS quality sigma_overall_arcsec not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality sigma_overall_arcsec not available for comparison (2nd new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (2nd new image new=N/A ref_avg=N/A)
###################################
# 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 00:00:00.911 +30:00:05.90
Second-epoch second image center 00:00:01.372 +30:00:25.10
Angular distance between the image centers 0.00559 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits &> /tmp/tmp.sXu2w3l7a9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits &> /tmp/tmp.AGpCAgYHQQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits &> /tmp/tmp.rYlZMvRXxI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits &> /tmp/tmp.gbrPZitfvx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.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-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits and wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat
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-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits and wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat
Found non-empty wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits and wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat
The reference image (wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits) and catalog (wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat) found
'wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat' -> 'wcsmag.cat'
Read 77944 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0005 to 359.9996 deg, Dec +24.3227 to +35.3101 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 0.0005 to 359.9996 deg, Dec 24.3227 to 35.3101 deg
Loaded 205113 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): 5976 out of 7053 total matches.
Matched with Tycho-2 7053 out of 77944 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.837900
a=0.000000 b=1.000000 c=22.837900
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 77944 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0005 to 359.9996 deg, Dec +24.3227 to +35.3101 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 0.0005 to 359.9996 deg, Dec 24.3227 to 35.3101 deg
Loaded 205113 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): 5976 out of 7053 total matches.
Matched with Tycho-2 7053 out of 77944 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits:
Forced-photometry filter: calibrated wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits -> calib.txt_param_ref_wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits (aperture=4.7)
Read 73343 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9999 deg, Dec +24.2877 to +35.2820 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 0.0002 to 359.9999 deg, Dec 24.2877 to 35.2820 deg
Loaded 205203 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): 44 out of 55 total matches.
Matched with Tycho-2 55 out of 73343 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits:
Forced-photometry filter: calibrated wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits -> calib.txt_param_ref_wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 74 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
1.9 pix Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
2.3 pix fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
2.3 pix fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
1.9 pix wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
1.9 pix wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Limiting magnitude estimates:
15.6 mag. Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
15.5 mag. Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
14.8 mag. fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
14.8 mag. fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.2 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.sXu2w3l7a9 (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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.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-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits' -> 'wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
WCS_IMAGE_NAME=wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
WCS-calibrated image found: wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
Checking if the catalog wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits alredy exist and is non-empty...
Catalog wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits
WCS catalog name: wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=4886, passed=77924
Got 77924 stars (including 72904 good ones) from the SExtractor catalog wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat
util/solve_plate_with_UCAC5 got 77924 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.5829 through 0 to 9.6840, gap 9.6840 to 350.5829
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 76624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 350.5823 through 0 to 9.6845, gap 9.6845 to 350.5823
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 76624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 76623 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits N_match=968 sigma_overall_arcsec=0.334 sigma_q1_arcsec=0.414 sigma_q2_arcsec=0.316 sigma_q3_arcsec=0.332 sigma_q4_arcsec=0.306 n_q1=219 n_q2=258 n_q3=242 n_q4=249 worst_quadrant_to_overall_ratio=1.241
The image catalog is written to wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits -region wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.AGpCAgYHQQ (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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.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-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits' -> 'wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
WCS-calibrated image found: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
Checking if the catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat corresponding to the image wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits
WCS catalog name: wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=4370, passed=73327
Got 73327 stars (including 68839 good ones) from the SExtractor catalog wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat
util/solve_plate_with_UCAC5 got 73327 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.4'
Seting catalog search parameters based on the expected field of view 931.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012936 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010349 (37.3 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 350.8529 through 0 to 9.7454, gap 9.7454 to 350.8529
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 198 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 171 matched stars entering correct_measured_positions(), 138 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 165 matched stars entering correct_measured_positions(), 13564 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.76"
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 350.8530 through 0 to 9.7396, gap 9.7396 to 350.8530
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 250 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 225 matched stars entering correct_measured_positions(), 13588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.76"
Accuracy estimation diagnostic: 224 matched stars entering correct_measured_positions(), 18001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.94"
Excluding outliers - 224 stars left (next iteration limit 181)
WCS_QUALITY_DIAG: file=Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits N_match=224 sigma_overall_arcsec=11.232 sigma_q1_arcsec=7.263 sigma_q2_arcsec=23.562 sigma_q3_arcsec=19.306 sigma_q4_arcsec=26.224 n_q1=139 n_q2=13 n_q3=66 n_q4=6 worst_quadrant_to_overall_ratio=2.335
The image catalog is written to wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits -region wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.rYlZMvRXxI (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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
WCS_IMAGE_NAME=wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
WCS-calibrated image found: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Checking if the catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
WCS catalog name: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=2295, passed=50090
Got 50090 stars (including 47717 good ones) from the SExtractor catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat
util/solve_plate_with_UCAC5 got 50090 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.7748 through 0 to 9.8696, gap 9.8696 to 350.7748
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 49367 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 350.7739 through 0 to 9.8695, gap 9.8695 to 350.7739
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 49368 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 49366 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits N_match=962 sigma_overall_arcsec=0.346 sigma_q1_arcsec=0.372 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.284 sigma_q4_arcsec=0.330 n_q1=247 n_q2=208 n_q3=273 n_q4=234 worst_quadrant_to_overall_ratio=1.075
The image catalog is written to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits -region wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.gbrPZitfvx (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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
WCS_IMAGE_NAME=wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
WCS-calibrated image found: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Checking if the catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat corresponding to the image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
WCS catalog name: wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=2177, passed=50370
Got 50370 stars (including 48114 good ones) from the SExtractor catalog wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat
util/solve_plate_with_UCAC5 got 50370 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 350.7748 through 0 to 9.8699, gap 9.8699 to 350.7748
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 49646 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 350.7739 through 0 to 9.8698, gap 9.8698 to 350.7739
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 49644 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 49644 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits N_match=961 sigma_overall_arcsec=0.343 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.359 sigma_q3_arcsec=0.310 sigma_q4_arcsec=0.370 n_q1=248 n_q2=211 n_q3=272 n_q4=230 worst_quadrant_to_overall_ratio=1.079
The image catalog is written to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits -region wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-09-57_20.00sec_-4.90C_LIGHTs_0438.fits
Saving fully-calibrated image wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.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_2026-05-13_CI_Peg-01-Q1b1x1_061434_TTUQ1b1x1_3987756_EWqX7oEF/wcs_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439.fits
Preparing the HTML report for the field Peg-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:35:41.25 +25:33:04.1: 13.64 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:54:23.65 +28:05:04.6: 13.96 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:48:59.83 +28:45:20.6: 14.13 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:29:44.49 +31:50:01.0: 13.72 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:29:41.06 +28:56:38.9: 13.28 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:37:27.57 +32:29:08.2: 14.34 +/- 0.08 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:47:37.30 +34:46:21.1: 13.59 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:44:27.09 +32:40:25.3: 13.63 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:35:41.25 +25:33:04.1: 15.45 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry filter REJECTED candidate at 23:35:41.25 +25:33:04.1: ref_mag=13.69 +/- 0.04 new_mean_mag=13.8361 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:29:44.49 +31:50:01.0: 12.82 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:54:23.65 +28:05:04.6: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:48:59.83 +28:45:20.6: 16.01 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter REJECTED candidate at 23:54:23.65 +28:05:04.6: ref_mag=13.96 +/- 0.04 new_mean_mag=13.8850 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:29:44.49 +31:50:01.0: ref_mag=13.06 +/- 0.02 new_mean_mag=13.8701 delta=-0.81 (need > 0.90)
Forced photometry reference-image weighted average: 14.13 +/- 0.05
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:33:26.15 +27:15:35.8: 12.90 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 23:48:59.83 +28:45:20.6: ref_mag=14.13 +/- 0.05 new_mean_mag=14.2649 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:44:27.09 +32:40:25.3: 14.96 +/- 0.15 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:37:27.57 +32:29:08.2: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:29:41.06 +28:56:38.9: 15.78 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry reference-image weighted average: 14.34 +/- 0.08
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:47:37.30 +34:46:21.1: 15.79 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 23:44:27.09 +32:40:25.3: ref_mag=13.71 +/- 0.03 new_mean_mag=14.1110 delta=-0.41 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:37:27.57 +32:29:08.2: ref_mag=14.34 +/- 0.08 new_mean_mag=14.3835 delta=-0.05 (need > 0.90)
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Forced photometry filter REJECTED candidate at 23:29:41.06 +28:56:38.9: ref_mag=13.28 +/- 0.03 new_mean_mag=13.4390 delta=-0.16 (need > 0.90)
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Forced photometry filter REJECTED candidate at 23:47:37.30 +34:46:21.1: ref_mag=13.59 +/- 0.04 new_mean_mag=13.6924 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:32:27.17 +30:16:32.4: 12.67 +/- 0.02 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:33:26.15 +27:15:35.8: 15.72 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry filter REJECTED candidate at 23:33:26.15 +27:15:35.8: ref_mag=12.90 +/- 0.02 new_mean_mag=12.9737 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:32:27.17 +30:16:32.4: 15.81 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.67 +/- 0.02
Forced photometry filter REJECTED candidate at 23:32:27.17 +30:16:32.4: ref_mag=12.67 +/- 0.02 new_mean_mag=12.7827 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:57:52.34 +25:06:30.2: 12.63 +/- 0.02 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:47:46.96 +31:15:54.6: 13.40 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:33:02.96 +32:15:48.0: 13.24 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:06:42.17 +28:32:28.2: 13.25 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:13:46.25 +34:51:22.4: 13.39 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:57:52.34 +25:06:30.2: 15.87 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Forced photometry filter REJECTED candidate at 23:57:52.34 +25:06:30.2: ref_mag=12.63 +/- 0.02 new_mean_mag=12.6634 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:10:44.50 +32:12:26.6: 13.56 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:42:18.18 +32:28:50.5: 13.62 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:33:02.96 +32:15:48.0: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:06:42.17 +28:32:28.2: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:47:46.96 +31:15:54.6: 16.02 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Forced photometry filter REJECTED candidate at 23:33:02.96 +32:15:48.0: ref_mag=13.24 +/- 0.03 new_mean_mag=13.4937 delta=-0.26 (need > 0.90)
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:48:22.63 +30:31:10.6: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Forced photometry filter REJECTED candidate at 00:06:42.17 +28:32:28.2: ref_mag=13.25 +/- 0.03 new_mean_mag=13.1413 delta=0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:47:46.96 +31:15:54.6: ref_mag=13.40 +/- 0.03 new_mean_mag=13.2886 delta=0.12 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:06:36.16 +27:05:57.9: 13.69 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:13:46.25 +34:51:22.4: 15.13 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Forced photometry filter REJECTED candidate at 00:13:46.25 +34:51:22.4: ref_mag=13.44 +/- 0.04 new_mean_mag=13.3713 delta=0.07 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:43:44.78 +30:44:29.1: 13.65 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:10:44.50 +32:12:26.6: 15.49 +/- 0.28 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.04
Forced photometry filter REJECTED candidate at 00:10:44.50 +32:12:26.6: ref_mag=13.60 +/- 0.04 new_mean_mag=13.4297 delta=0.17 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:42:18.18 +32:28:50.5: 15.96 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.62 +/- 0.04
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:48:22.63 +30:31:10.6: 16.02 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 23:42:18.18 +32:28:50.5: ref_mag=13.62 +/- 0.04 new_mean_mag=13.5962 delta=0.03 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:06:36.16 +27:05:57.9: 15.84 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.53 +/- 0.04
Forced photometry filter REJECTED candidate at 23:48:22.63 +30:31:10.6: ref_mag=13.53 +/- 0.04 new_mean_mag=13.4745 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry filter REJECTED candidate at 00:06:36.16 +27:05:57.9: ref_mag=13.69 +/- 0.04 new_mean_mag=13.4816 delta=0.21 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:43:44.78 +30:44:29.1: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter REJECTED candidate at 23:43:44.78 +30:44:29.1: ref_mag=13.71 +/- 0.03 new_mean_mag=13.5958 delta=0.11 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:35:40.02 +34:14:47.0: 13.65 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:29:21.62 +30:25:08.1: 13.44 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:37:32.01 +30:17:00.9: 13.77 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:35:40.02 +34:14:47.0: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:59:58.43 +25:52:53.3: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Forced photometry filter REJECTED candidate at 23:35:40.02 +34:14:47.0: ref_mag=13.65 +/- 0.04 new_mean_mag=13.6996 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:10:38.60 +32:15:43.5: 13.59 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:58:13.06 +29:58:39.4: 13.70 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:29:21.62 +30:25:08.1: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:37:32.01 +30:17:00.9: 15.88 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Forced photometry filter REJECTED candidate at 23:29:21.62 +30:25:08.1: ref_mag=13.44 +/- 0.04 new_mean_mag=13.6237 delta=-0.19 (need > 0.90)
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Forced photometry filter REJECTED candidate at 23:37:32.01 +30:17:00.9: ref_mag=13.77 +/- 0.04 new_mean_mag=13.8171 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:08:08.56 +29:43:13.1: 13.84 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:00:05.88 +25:51:50.1: 13.25 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:59:58.43 +25:52:53.3: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:47:16.04 +31:52:41.1: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.04
Forced photometry filter REJECTED candidate at 23:59:58.43 +25:52:53.3: ref_mag=13.51 +/- 0.04 new_mean_mag=13.6878 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:10:38.60 +32:15:43.5: 15.77 +/- 0.34 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:32:46.26 +27:07:11.1: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.04
Forced photometry filter REJECTED candidate at 00:10:38.60 +32:15:43.5: ref_mag=13.62 +/- 0.04 new_mean_mag=13.7130 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:00:05.88 +25:51:50.1: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:08:08.56 +29:43:13.1: 15.93 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:58:13.06 +29:58:39.4: 15.82 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 00:00:05.88 +25:51:50.1: ref_mag=13.25 +/- 0.03 new_mean_mag=13.7286 delta=-0.48 (need > 0.90)
Forced photometry reference-image weighted average: 13.84 +/- 0.04
Forced photometry filter REJECTED candidate at 00:08:08.56 +29:43:13.1: ref_mag=13.84 +/- 0.04 new_mean_mag=13.7266 delta=0.11 (need > 0.90)
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Forced photometry filter REJECTED candidate at 23:58:13.06 +29:58:39.4: ref_mag=13.70 +/- 0.04 new_mean_mag=13.7305 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:17:56.83 +34:35:30.5: 13.70 +/- 0.04 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:47:16.04 +31:52:41.1: 15.95 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.85 +/- 0.05
Forced photometry filter REJECTED candidate at 23:47:16.04 +31:52:41.1: ref_mag=13.85 +/- 0.05 new_mean_mag=13.8623 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:41:20.74 +32:34:36.0: 13.89 +/- 0.06 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:32:46.26 +27:07:11.1: 14.85 +/- 0.17 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:51:45.15 +30:35:32.2: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.05
Forced photometry filter REJECTED candidate at 23:32:46.26 +27:07:11.1: ref_mag=13.92 +/- 0.05 new_mean_mag=13.9111 delta=0.01 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:17:56.83 +34:35:30.5: 15.75 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Forced photometry filter REJECTED candidate at 00:17:56.83 +34:35:30.5: ref_mag=13.70 +/- 0.04 new_mean_mag=13.7107 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:06:56.79 +31:08:02.8: 13.97 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:15:04.52 +34:52:45.8: 13.89 +/- 0.06 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:53:13.83 +34:30:15.0: 13.93 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:51:45.15 +30:35:32.2: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:41:20.74 +32:34:36.0: 15.91 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.78 +/- 0.05
Forced photometry reference-image weighted average: 13.89 +/- 0.06
Forced photometry filter REJECTED candidate at 23:41:20.74 +32:34:36.0: ref_mag=13.89 +/- 0.06 new_mean_mag=13.9768 delta=-0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:51:45.15 +30:35:32.2: ref_mag=13.78 +/- 0.05 new_mean_mag=13.7209 delta=0.05 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:26:47.44 +27:58:56.9: 13.82 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:31:41.01 +28:13:24.4: 14.07 +/- 0.07 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:06:56.79 +31:08:02.8: 12.03 +/- 0.01 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:15:04.52 +34:52:45.8: 15.70 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Forced photometry filter REJECTED candidate at 00:06:56.79 +31:08:02.8: ref_mag=12.12 +/- 0.01 new_mean_mag=13.9417 delta=-1.82 (need > 0.90)
Forced photometry reference-image weighted average: 13.89 +/- 0.06
Forced photometry filter REJECTED candidate at 00:15:04.52 +34:52:45.8: ref_mag=13.89 +/- 0.06 new_mean_mag=13.9333 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:53:13.83 +34:30:15.0: 15.94 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.93 +/- 0.05
Forced photometry filter REJECTED candidate at 23:53:13.83 +34:30:15.0: ref_mag=13.93 +/- 0.05 new_mean_mag=13.9971 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:45:32.49 +31:55:07.3: 14.22 +/- 0.06 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:26:47.44 +27:58:56.9: 15.79 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Forced photometry filter REJECTED candidate at 00:26:47.44 +27:58:56.9: ref_mag=13.82 +/- 0.05 new_mean_mag=13.7701 delta=0.05 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:31:41.01 +28:13:24.4: 15.78 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.07 +/- 0.07
Forced photometry filter REJECTED candidate at 23:31:41.01 +28:13:24.4: ref_mag=14.07 +/- 0.07 new_mean_mag=14.1977 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:07:27.99 +26:27:54.6: 13.86 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:55:11.24 +28:39:03.5: 14.23 +/- 0.07 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:47:36.30 +29:02:30.3: 14.34 +/- 0.07 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:09:05.59 +34:21:47.5: 14.10 +/- 0.07 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:45:32.49 +31:55:07.3: 15.94 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.22 +/- 0.06
Forced photometry filter REJECTED candidate at 23:45:32.49 +31:55:07.3: ref_mag=14.22 +/- 0.06 new_mean_mag=14.1542 delta=0.07 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:27:29.95 +29:45:08.0: 14.61 +/- 0.10 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:53:23.29 +28:57:45.0: 14.16 +/- 0.05 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:07:27.99 +26:27:54.6: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:47:36.30 +29:02:30.3: 15.94 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.34 +/- 0.07
Forced photometry reference-image weighted average: 13.86 +/- 0.05
Forced photometry filter REJECTED candidate at 23:47:36.30 +29:02:30.3: ref_mag=14.34 +/- 0.07 new_mean_mag=14.1731 delta=0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:07:27.99 +26:27:54.6: ref_mag=13.86 +/- 0.05 new_mean_mag=14.0525 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:09:05.59 +34:21:47.5: 12.88 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:55:11.24 +28:39:03.5: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:41:37.66 +29:08:32.4: 15.00 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.07
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter REJECTED candidate at 00:09:05.59 +34:21:47.5: ref_mag=13.05 +/- 0.02 new_mean_mag=14.2492 delta=-1.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:55:11.24 +28:39:03.5: ref_mag=14.23 +/- 0.07 new_mean_mag=14.1333 delta=0.10 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:31:36.69 +32:39:30.7: 15.05 +/- 0.16 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:53:23.29 +28:57:45.0: 15.29 +/- 0.18 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:41:37.66 +29:08:32.4: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:54:00.20 +28:28:16.9: 15.17 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.00 +/- 0.13
Forced photometry filter REJECTED candidate at 23:41:37.66 +29:08:32.4: ref_mag=15.00 +/- 0.13 new_mean_mag=14.6371 delta=0.37 (need > 0.90)
Forced photometry reference-image weighted average: 14.24 +/- 0.05
Forced photometry filter REJECTED candidate at 23:53:23.29 +28:57:45.0: ref_mag=14.24 +/- 0.05 new_mean_mag=14.3460 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:27:29.95 +29:45:08.0: 15.69 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.61 +/- 0.10
Forced photometry filter REJECTED candidate at 23:27:29.95 +29:45:08.0: ref_mag=14.61 +/- 0.10 new_mean_mag=14.4605 delta=0.15 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:31:36.69 +32:39:30.7: 15.78 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.05 +/- 0.16
Forced photometry filter REJECTED candidate at 23:31:36.69 +32:39:30.7: ref_mag=15.05 +/- 0.16 new_mean_mag=14.8521 delta=0.20 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:54:00.20 +28:28:16.9: 15.97 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.17 +/- 0.15
Forced photometry filter REJECTED candidate at 23:54:00.20 +28:28:16.9: ref_mag=15.17 +/- 0.15 new_mean_mag=14.8790 delta=0.29 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 00:27:14.15 +30:53:48.0: 13.44 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2025-12-22_21-35-58_20.00sec_-15.00C_LIGHT_0123.fits at 23:51:44.08 +29:45:43.3: 13.25 +/- 0.03 detection
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 00:27:14.15 +30:53:48.0: 14.28 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.54 +/- 0.03
Forced photometry filter KEPT candidate at 00:27:14.15 +30:53:48.0: ref_mag=13.54 +/- 0.03 new_mean_mag=10.6390 delta=2.90 (need > 0.90)
Forced photometry on wcs_Peg-01-Q1b1x1_2026-01-08_20-58-42_20.00sec_-15.00C_LIGHT_0071.fits at 23:51:44.08 +29:45:43.3: 16.07 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.25 +/- 0.03
Forced photometry filter KEPT candidate at 23:51:44.08 +29:45:43.3: ref_mag=13.25 +/- 0.03 new_mean_mag=10.3368 delta=2.91 (need > 0.90)
Adding exclusion_list_local.txt__out33513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44696.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
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 91518_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91518_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91523_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91523_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91526_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91526_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91527_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91527_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91529_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91529_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91530_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91530_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91531_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91531_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91534_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91534_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 00:06:59.04 +25:51:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91535_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91535_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 23:28:10.96 +25:55:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91536_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91536_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91537_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91537_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 00:29:25.40 +24:40:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91538_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91538_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91539_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91539_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91627_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91627_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 91646_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91646_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 91671_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91671_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 23:49:33.56 +28:51:34.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 91727_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91727_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 23:24:43.89 +32:24:37.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 91738_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91738_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 91740_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91740_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91785_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91785_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 91861_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91861_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 23:34:01.76 +31:21:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91864_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91864_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91871_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91871_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 23:33:58.75 +31:54:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91887_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91887_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91890_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91890_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 91900_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91900_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 91928_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91928_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91947_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91947_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91954_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91954_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91958_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91958_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91961_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91961_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91984_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91984_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 91998_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 91998_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92006_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92006_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92008_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92008_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 23:39:47.09 +34:58:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92019_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92019_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92048_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92048_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92050_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92050_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 92056_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92056_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92065_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92065_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 92071_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92071_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92090_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92090_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92097_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92097_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92099_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92099_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92109_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92109_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92122_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92122_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92143_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92143_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92151_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92151_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92160_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92160_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92169_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92169_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 23:46:15.96 +34:11:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92218_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92218_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92230_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92230_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 92233_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92233_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92250_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92250_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92295_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92295_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92328_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92328_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92346_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92346_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92354_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92354_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 00:12:01.79 +25:48:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92411_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92411_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92417_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92417_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92433_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92433_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92492_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92492_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92498_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92498_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92546_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92546_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92582_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92582_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92596_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92596_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 92618_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92618_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 92625_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 92625_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
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Considering the candidate 66971_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 66971_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 00:22:23.13 +26:59:46.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 48992_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 48992_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 00:14:10.89 +29:01:20.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 21084_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 21084_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
**** FOUND 23:36:59.63 +32:42:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33513_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
Preparing report for the candidate 33513_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
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Considering the candidate 66096_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439
The candidate 66096_fd_Peg-01-Q1b1x1_2026-05-13_05-10-36_20.00sec_-5.00C_LIGHTs_0439 did not pass the final checks
