This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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
RU Peg,2461271.8788,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RU Peg 20260819.3788 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 19.3788 2461271.8788 12.55 22:15:12.33 +13:40:53.1
75.10084 -34.30671 galactic Peg Second-epoch detections are separated by 0.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.225 Henrietta 0 -0 0 12.6 -0 0
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:15:12.33 +13:40:53.1: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:15:12.33 +13:40:53.1: 16.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461271.8788,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260819.3788 12.55CV 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 08 19.3788 2461271.8788 14.24 22:07:32.31 +12:53:51.8
72.82113 -33.58717 galactic Peg Second-epoch detections are separated by 0.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1031 Arctica -1 -1 1 14.4 -0 0
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:07:32.31 +12:53:51.8: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:07:32.31 +12:53:51.8: 16.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461271.8788,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260819.3788 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 19.3788 2461271.8788 14.77 22:26:32.11 +12:51:04.2
76.94124 -36.76583 galactic Peg Second-epoch detections are separated by 0.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.2771 Polzunov -0 0 0 15.2 0 0
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:26:32.11 +12:51:04.2: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:26:32.11 +12:51:04.2: 15.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461271.8788,14.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260819.3788 14.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RU Peg,2461271.8788,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RU Peg 20260819.3788 10.37CV 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: 2461208.85737810 17.06.2026 08:34:27.468 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
First image: 2461208.85737810 17.06.2026 08:34:27.468 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
Last image: 2461271.87916830 19.08.2026 09:05:50.141 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 9198
Objects passed selection criteria: 9193
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 8953.75
Average stars matched: 7945 (88.7338 %)
Memory usage VmPeak: 236132 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Aug 19 04:18:10 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: 2461208.85737810 17.06.2026 08:34:27.468 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
First image: 2461208.85737810 17.06.2026 08:34:27.468 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
Last image: 2461271.87916830 19.08.2026 09:05:50.141 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 84
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
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: 35 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 56296
Objects passed selection criteria: 56167
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 55786.2
Average stars matched: 49996.5 (89.6215 %)
Memory usage VmPeak: 281216 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Aug 19 04:19:31 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
SExtractor catalog cache: saved Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.cat to cache
SExtractor catalog cache: saved Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.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-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.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: 2461271.87839080
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits exists and is non-empty
wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits exists and is non-empty
wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits exists and is non-empty
wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits (1st reference image)
verification OK: wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:13:23.871 +14:00:53.76 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits (1st new image)
verification OK: wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:13:20.716 +13:58:41.37 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:13:23.871 +14:00:53.76
Second-epoch image center 22:13:20.716 +13:58:41.37
Angular distance between the image centers 0.0389 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits (2nd new image)
verification OK: wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:13:18.421 +13:59:05.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:13:23.871 +14:00:53.76
Second-epoch image center 22:13:18.421 +13:59:05.43
Angular distance between the image centers 0.0373 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:13:20.716 +13:58:41.37
Second-epoch second image center 22:13:18.421 +13:59:05.43
Angular distance between the image centers 0.01144 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits &> /tmp/tmp.CPXae90Oxm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits &> /tmp/tmp.h28RRcc8Aw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits &> /tmp/tmp.GjQ10hiBez
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits &> /tmp/tmp.MOpn09Oekd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.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-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits and wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits and wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat
Found non-empty wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits and wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat
The reference image (wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits) and catalog (wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat) found
'wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat' -> 'wcsmag.cat'
Read 10872 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.0562 to 341.5470 deg, Dec +8.6476 to +19.2847 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 325.0562 to 341.5470 deg, Dec 8.6476 to 19.2847 deg
Loaded 7933 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): 6465 out of 6670 total matches.
Matched with Tycho-2 6670 out of 10872 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.709600
a=0.000000 b=1.000000 c=22.709600
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.09
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 10872 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.0562 to 341.5470 deg, Dec +8.6476 to +19.2847 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 325.0562 to 341.5470 deg, Dec 8.6476 to 19.2847 deg
Loaded 7933 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): 6465 out of 6670 total matches.
Matched with Tycho-2 6670 out of 10872 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
Forced-photometry filter: calibrated wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits -> calib.txt_param_ref_wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits (aperture=6.2)
Read 11441 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.0622 to 341.5504 deg, Dec +8.6947 to +19.2751 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 325.0622 to 341.5504 deg, Dec 8.6947 to 19.2751 deg
Loaded 7885 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): 6468 out of 6725 total matches.
Matched with Tycho-2 6725 out of 11441 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
Forced-photometry filter: calibrated wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits -> calib.txt_param_ref_wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
2.3 pix Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
2.4 pix fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
2.3 pix fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
Limiting magnitude estimates:
15.1 mag. Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
15.2 mag. Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
15.2 mag. fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
15.2 mag. fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.CPXae90Oxm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.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-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits' -> 'wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
WCS_IMAGE_NAME=wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
WCS-calibrated image found: wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
Checking if the catalog wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat corresponding to the image wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits alredy exist and is non-empty...
Catalog wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat corresponding to the image wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
WCS catalog name: wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=579, bad_region=2343, passed=10872
Got 10872 stars (including 8048 good ones) from the SExtractor catalog wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat
util/solve_plate_with_UCAC5 got 10872 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4671 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4641 matched stars entering correct_measured_positions(), 4641 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4641 matched stars entering correct_measured_positions(), 9002 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4671 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4641 matched stars entering correct_measured_positions(), 9002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4641 matched stars entering correct_measured_positions(), 9002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4641 stars left (next iteration limit 5105)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits N_match=4641 sigma_overall_arcsec=0.369 sigma_q1_arcsec=0.333 sigma_q2_arcsec=0.360 sigma_q3_arcsec=0.420 sigma_q4_arcsec=0.360 n_q1=1430 n_q2=750 n_q3=1568 n_q4=893 worst_quadrant_to_overall_ratio=1.138
The image catalog is written to wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits -region wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.h28RRcc8Aw (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.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-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits' -> 'wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
WCS_IMAGE_NAME=wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
WCS-calibrated image found: wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
Checking if the catalog wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat corresponding to the image wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits alredy exist and is non-empty...
Catalog wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat corresponding to the image wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
WCS catalog name: wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=656, bad_region=2966, passed=11441
Got 11441 stars (including 7944 good ones) from the SExtractor catalog wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat
util/solve_plate_with_UCAC5 got 11441 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4691 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4664 matched stars entering correct_measured_positions(), 4665 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4664 matched stars entering correct_measured_positions(), 9078 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4691 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4664 matched stars entering correct_measured_positions(), 9078 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4664 matched stars entering correct_measured_positions(), 9078 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4664 stars left (next iteration limit 5130)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits N_match=4664 sigma_overall_arcsec=0.408 sigma_q1_arcsec=0.361 sigma_q2_arcsec=0.432 sigma_q3_arcsec=0.462 sigma_q4_arcsec=0.411 n_q1=1513 n_q2=1025 n_q3=1269 n_q4=857 worst_quadrant_to_overall_ratio=1.131
The image catalog is written to wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits -region wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GjQ10hiBez (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
Checking if the catalog wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
WCS catalog name: wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=627, bad_region=2911, passed=12569
Got 12569 stars (including 9153 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat
util/solve_plate_with_UCAC5 got 12569 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 4693 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4667 matched stars entering correct_measured_positions(), 4667 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4667 matched stars entering correct_measured_positions(), 10288 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 4693 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4667 matched stars entering correct_measured_positions(), 10288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4667 matched stars entering correct_measured_positions(), 10288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4667 stars left (next iteration limit 5133)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4667 robust_rms=6.866 arcsec worst_quadrant_rms=8.093 arcsec
SIP_REFIT: SIP order 3 trial: matched=4667 robust_rms=0.326 arcsec worst_quadrant_rms=0.360 arcsec
SIP_REFIT: SIP order 5 trial: matched=4667 robust_rms=0.282 arcsec worst_quadrant_rms=0.303 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4667 robust_rms_before=0.657 arcsec robust_rms_before_corrected=0.295 arcsec robust_rms_after=0.282 arcsec worst_quadrant_rms_before=0.334 worst_quadrant_rms_after=0.303
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.334 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits N_match=4667 sigma_overall_arcsec=0.295 sigma_q1_arcsec=0.280 sigma_q2_arcsec=0.300 sigma_q3_arcsec=0.288 sigma_q4_arcsec=0.333 n_q1=1538 n_q2=1004 n_q3=1286 n_q4=839 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits -region wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MOpn09Oekd (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
Checking if the catalog wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
WCS catalog name: wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=714, bad_region=2962, passed=12303
Got 12303 stars (including 8809 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat
util/solve_plate_with_UCAC5 got 12303 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 4692 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4664 matched stars entering correct_measured_positions(), 4664 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4664 matched stars entering correct_measured_positions(), 9992 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 4692 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4664 matched stars entering correct_measured_positions(), 9992 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4664 matched stars entering correct_measured_positions(), 9992 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4664 stars left (next iteration limit 5130)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4664 robust_rms=6.844 arcsec worst_quadrant_rms=8.246 arcsec
SIP_REFIT: SIP order 3 trial: matched=4664 robust_rms=0.376 arcsec worst_quadrant_rms=0.427 arcsec
SIP_REFIT: SIP order 5 trial: matched=4664 robust_rms=0.334 arcsec worst_quadrant_rms=0.352 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4664 robust_rms_before=0.672 arcsec robust_rms_before_corrected=0.337 arcsec robust_rms_after=0.334 arcsec worst_quadrant_rms_before=0.377 worst_quadrant_rms_after=0.352
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.377 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits N_match=4664 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.332 sigma_q2_arcsec=0.363 sigma_q3_arcsec=0.366 sigma_q4_arcsec=0.383 n_q1=1536 n_q2=1000 n_q3=1286 n_q4=842 worst_quadrant_to_overall_ratio=1.066
The image catalog is written to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits -region wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits to local_wcs_cache/
'wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits' -> 'local_wcs_cache/wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits'
Saving the final (post-refit) wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits to local_wcs_cache/
'wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits' -> 'local_wcs_cache/wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits'
Saving the final (post-refit) wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits to local_wcs_cache/
'wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits' -> 'local_wcs_cache/wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits'
Saving the final (post-refit) wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits to local_wcs_cache/
'wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits' -> 'local_wcs_cache/wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits sigma_overall=0.369 worst_q_ratio=1.138
ref2=Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits sigma_overall=0.408 worst_q_ratio=1.131
new1=fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits sigma_overall=0.295 worst_q_ratio=1.130
new2=fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits sigma_overall=0.359 worst_q_ratio=1.066
reference average sigma_overall=0.3885 worst_q_ratio=1.1345
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368_astrometric_residuals.png (4641 matched stars from wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471_astrometric_residuals.png (4664 matched stars from wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414_astrometric_residuals.png (4667 matched stars from wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415_astrometric_residuals.png (4664 matched stars from wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits'
Saving fully-calibrated image wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits'
Preparing the HTML report for the field Peg-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:11:08.82 +14:59:43.4: 12.16 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:28:32.80 +16:07:23.3: 10.84 +/- 0.00 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:12:19.95 +13:23:44.8: 12.23 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:06:02.01 +14:43:21.6: 12.24 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:14:35.10 +16:41:40.4: 12.13 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:10:35.42 +13:34:20.6: 12.05 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:16:35.43 +14:45:04.6: 12.14 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:06:02.01 +14:43:21.6: 12.21 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:14:35.10 +16:41:40.4: 12.17 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:16:35.43 +14:45:04.6: 12.14 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:11:08.82 +14:59:43.4: 12.21 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:28:32.80 +16:07:23.3: 10.81 +/- 0.00 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:10:35.42 +13:34:20.6: 12.04 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:12:19.95 +13:23:44.8: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry filter REJECTED candidate at 22:06:02.01 +14:43:21.6: ref_mag=12.22 +/- 0.01 new_mean_mag=12.1908 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:14:35.10 +16:41:40.4: ref_mag=12.15 +/- 0.01 new_mean_mag=12.1795 delta=-0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:28:32.80 +16:07:23.3: ref_mag=10.83 +/- 0.00 new_mean_mag=11.1007 delta=-0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:16:35.43 +14:45:04.6: ref_mag=12.14 +/- 0.01 new_mean_mag=12.1368 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:11:08.82 +14:59:43.4: ref_mag=12.19 +/- 0.01 new_mean_mag=12.1935 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:10:35.42 +13:34:20.6: ref_mag=12.04 +/- 0.01 new_mean_mag=12.0408 delta=0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:12:19.95 +13:23:44.8: ref_mag=12.24 +/- 0.01 new_mean_mag=12.2141 delta=0.03 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22643_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 22643_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22649_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 22649_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
**** FOUND 22:03:33.95 +14:00:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22658_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 22658_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22659_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 22659_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22660_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 22660_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22661_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 22661_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22663_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 22663_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22664_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 22664_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21208_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 21208_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
**** FOUND 22:11:37.48 +14:21:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03891_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
Preparing report for the candidate 03891_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Peg-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
SExtractor catalog cache: saved Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.cat to cache
SExtractor catalog cache: saved Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.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-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
Creating symlink local_wcs_cache/wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits exists and is non-empty
wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits exists and is non-empty
wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits exists and is non-empty
wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits (1st reference image)
verification OK: wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:13:23.871 +14:00:53.76 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits (1st new image)
verification OK: wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:13:20.716 +13:58:41.37 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:13:23.871 +14:00:53.76
Second-epoch image center 22:13:20.716 +13:58:41.37
Angular distance between the image centers 0.0389 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits (2nd new image)
verification OK: wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:13:18.421 +13:59:05.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:13:23.871 +14:00:53.76
Second-epoch image center 22:13:18.421 +13:59:05.43
Angular distance between the image centers 0.0373 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:13:20.716 +13:58:41.37
Second-epoch second image center 22:13:18.421 +13:59:05.43
Angular distance between the image centers 0.01144 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits &> /tmp/tmp.6Z7f4OAehV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits &> /tmp/tmp.7HS9CFD955
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits &> /tmp/tmp.v1JYzfqiZP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits &> /tmp/tmp.uzz57A3EQy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.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-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits and wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits and wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat
Found non-empty wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits and wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat
The reference image (wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits) and catalog (wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat) found
'wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat' -> 'wcsmag.cat'
Read 66519 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.0563 to 341.5469 deg, Dec +8.6259 to +19.2851 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 325.0563 to 341.5469 deg, Dec 8.6259 to 19.2851 deg
Loaded 7951 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): 6095 out of 6879 total matches.
Matched with Tycho-2 6879 out of 66519 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.574300
a=0.000000 b=1.000000 c=22.574300
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.26
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 66519 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.0563 to 341.5469 deg, Dec +8.6259 to +19.2851 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 325.0563 to 341.5469 deg, Dec 8.6259 to 19.2851 deg
Loaded 7951 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): 6095 out of 6879 total matches.
Matched with Tycho-2 6879 out of 66519 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
Forced-photometry filter: calibrated wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits -> calib.txt_param_ref_wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits (aperture=4.8)
Read 73059 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 325.0608 to 341.5670 deg, Dec +8.6687 to +19.2801 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 325.0608 to 341.5670 deg, Dec 8.6687 to 19.2801 deg
Loaded 7919 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): 6034 out of 6894 total matches.
Matched with Tycho-2 6894 out of 73059 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
Forced-photometry filter: calibrated wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits -> calib.txt_param_ref_wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 61 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
2.1 pix Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
2.4 pix fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
2.2 pix fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
Limiting magnitude estimates:
15.3 mag. Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
15.4 mag. Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
15.3 mag. fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
15.4 mag. fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.6Z7f4OAehV (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.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-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits' -> 'wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
WCS_IMAGE_NAME=wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
WCS-calibrated image found: wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
Checking if the catalog wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat corresponding to the image wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits alredy exist and is non-empty...
Catalog wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat corresponding to the image wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits
WCS catalog name: wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=3884, bad_region=9359, passed=66496
Got 66496 stars (including 53784 good ones) from the SExtractor catalog wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat
util/solve_plate_with_UCAC5 got 66496 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4655 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4633 matched stars entering correct_measured_positions(), 4633 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4633 matched stars entering correct_measured_positions(), 59461 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4655 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4633 matched stars entering correct_measured_positions(), 59461 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4633 matched stars entering correct_measured_positions(), 59461 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4633 stars left (next iteration limit 5096)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits N_match=4633 sigma_overall_arcsec=0.367 sigma_q1_arcsec=0.331 sigma_q2_arcsec=0.358 sigma_q3_arcsec=0.418 sigma_q4_arcsec=0.355 n_q1=1438 n_q2=771 n_q3=1508 n_q4=916 worst_quadrant_to_overall_ratio=1.139
The image catalog is written to wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits -region wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.7HS9CFD955 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.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-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits' -> 'wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
WCS_IMAGE_NAME=wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
WCS-calibrated image found: wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
Checking if the catalog wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat corresponding to the image wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits alredy exist and is non-empty...
Catalog wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat corresponding to the image wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits
WCS catalog name: wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=4327, bad_region=15964, passed=73029
Got 73029 stars (including 53640 good ones) from the SExtractor catalog wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat
util/solve_plate_with_UCAC5 got 73029 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4686 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4669 matched stars entering correct_measured_positions(), 4670 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4669 matched stars entering correct_measured_positions(), 61057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4686 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4669 matched stars entering correct_measured_positions(), 61057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4669 matched stars entering correct_measured_positions(), 61057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4669 stars left (next iteration limit 5135)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits N_match=4669 sigma_overall_arcsec=0.401 sigma_q1_arcsec=0.363 sigma_q2_arcsec=0.437 sigma_q3_arcsec=0.442 sigma_q4_arcsec=0.403 n_q1=1512 n_q2=1010 n_q3=1273 n_q4=874 worst_quadrant_to_overall_ratio=1.103
The image catalog is written to wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits -region wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.v1JYzfqiZP (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
Checking if the catalog wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
WCS catalog name: wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=4563, bad_region=11597, passed=65747
Got 65747 stars (including 50893 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat
util/solve_plate_with_UCAC5 got 65747 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 4691 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4674 matched stars entering correct_measured_positions(), 4674 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4674 matched stars entering correct_measured_positions(), 57107 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 4690 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4674 matched stars entering correct_measured_positions(), 57107 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4674 matched stars entering correct_measured_positions(), 57107 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4674 stars left (next iteration limit 5141)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4674 robust_rms=6.828 arcsec worst_quadrant_rms=8.886 arcsec
SIP_REFIT: SIP order 3 trial: matched=4674 robust_rms=0.332 arcsec worst_quadrant_rms=0.357 arcsec
SIP_REFIT: SIP order 5 trial: matched=4674 robust_rms=0.284 arcsec worst_quadrant_rms=0.309 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4674 robust_rms_before=0.659 arcsec robust_rms_before_corrected=0.295 arcsec robust_rms_after=0.284 arcsec worst_quadrant_rms_before=0.348 worst_quadrant_rms_after=0.309
SIP_REFIT: applied the refit solution to the output catalog positions only (order 5, robust RMS 0.659 -> 0.284 arcsec); the image header was NOT rewritten as wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits is a symbolic link
WCS_QUALITY_DIAG: file=fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits N_match=4674 sigma_overall_arcsec=0.298 sigma_q1_arcsec=0.281 sigma_q2_arcsec=0.313 sigma_q3_arcsec=0.291 sigma_q4_arcsec=0.355 n_q1=1566 n_q2=960 n_q3=1322 n_q4=826 worst_quadrant_to_overall_ratio=1.193
The image catalog is written to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits -region wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.uzz57A3EQy (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
Checking if the catalog wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
WCS catalog name: wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=5093, bad_region=12031, passed=68284
Got 68284 stars (including 52916 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat
util/solve_plate_with_UCAC5 got 68284 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 4684 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4662 matched stars entering correct_measured_positions(), 4662 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4662 matched stars entering correct_measured_positions(), 59311 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.2)
Done reading UCAC5 zone files...
Matched 4684 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4662 matched stars entering correct_measured_positions(), 59311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4662 matched stars entering correct_measured_positions(), 59311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4662 stars left (next iteration limit 5128)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4662 robust_rms=6.819 arcsec worst_quadrant_rms=9.006 arcsec
SIP_REFIT: SIP order 3 trial: matched=4662 robust_rms=0.373 arcsec worst_quadrant_rms=0.423 arcsec
SIP_REFIT: SIP order 5 trial: matched=4662 robust_rms=0.327 arcsec worst_quadrant_rms=0.345 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4662 robust_rms_before=0.665 arcsec robust_rms_before_corrected=0.331 arcsec robust_rms_after=0.327 arcsec worst_quadrant_rms_before=0.372 worst_quadrant_rms_after=0.345
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.372 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits N_match=4662 sigma_overall_arcsec=0.346 sigma_q1_arcsec=0.324 sigma_q2_arcsec=0.355 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.371 n_q1=1562 n_q2=959 n_q3=1318 n_q4=823 worst_quadrant_to_overall_ratio=1.070
The image catalog is written to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits -region wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-04-42_20.00sec_-0.00C_LIGHT_0414.fits
Saving fully-calibrated image wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-19_CI_Peg-09-Q2b1x1_041530_TTUQ2b1x1_449460_LnFQrfGR/wcs_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415.fits
Preparing the HTML report for the field Peg-09-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:23:36.26 +17:18:00.3: 14.88 +/- 0.14 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:23:36.68 +11:51:35.6: 14.64 +/- 0.13 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:27:01.90 +12:33:28.8: 14.82 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:10:53.22 +13:09:46.2: 14.59 +/- 0.10 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:02:44.57 +11:13:09.7: 14.34 +/- 0.09 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:17:00.60 +17:55:50.5: 14.77 +/- 0.14 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:20:13.06 +18:08:11.0: 14.80 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:26:59.66 +10:30:24.0: 14.93 +/- 0.17 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:09:00.76 +17:42:56.4: 14.22 +/- 0.08 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:02:18.75 +10:58:47.0: 14.04 +/- 0.07 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:17:00.60 +17:55:50.5: 14.58 +/- 0.10 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:27:01.90 +12:33:28.8: 14.99 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:26:59.66 +10:30:24.0: 14.75 +/- 0.13 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:36.26 +17:18:00.3: 15.10 +/- 0.16 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:10:53.22 +13:09:46.2: 14.39 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.08
Forced photometry filter REJECTED candidate at 22:17:00.60 +17:55:50.5: ref_mag=14.65 +/- 0.08 new_mean_mag=14.6708 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 14.90 +/- 0.11
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:09:00.76 +17:42:56.4: 14.46 +/- 0.08 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:02:44.57 +11:13:09.7: 14.31 +/- 0.08 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:20:13.06 +18:08:11.0: 14.63 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.10
Forced photometry reference-image weighted average: 14.98 +/- 0.11
Forced photometry filter REJECTED candidate at 22:27:01.90 +12:33:28.8: ref_mag=14.90 +/- 0.11 new_mean_mag=14.7590 delta=0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:26:59.66 +10:30:24.0: ref_mag=14.81 +/- 0.10 new_mean_mag=14.7038 delta=0.11 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:02:18.75 +10:58:47.0: 14.32 +/- 0.09 detection
Forced photometry filter REJECTED candidate at 22:23:36.26 +17:18:00.3: ref_mag=14.98 +/- 0.11 new_mean_mag=14.8428 delta=0.13 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:36.68 +11:51:35.6: 14.71 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.06
Forced photometry reference-image weighted average: 14.69 +/- 0.09
Forced photometry reference-image weighted average: 14.46 +/- 0.06
Forced photometry filter REJECTED candidate at 22:02:44.57 +11:13:09.7: ref_mag=14.32 +/- 0.06 new_mean_mag=14.4644 delta=-0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:10:53.22 +13:09:46.2: ref_mag=14.46 +/- 0.06 new_mean_mag=14.7926 delta=-0.33 (need > 0.90)
Forced photometry reference-image weighted average: 14.15 +/- 0.06
Forced photometry reference-image weighted average: 14.33 +/- 0.06
Forced photometry filter REJECTED candidate at 22:20:13.06 +18:08:11.0: ref_mag=14.69 +/- 0.09 new_mean_mag=14.7999 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 14.68 +/- 0.09
Forced photometry filter REJECTED candidate at 22:09:00.76 +17:42:56.4: ref_mag=14.33 +/- 0.06 new_mean_mag=14.6655 delta=-0.34 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:02:18.75 +10:58:47.0: ref_mag=14.15 +/- 0.06 new_mean_mag=14.4768 delta=-0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:23:36.68 +11:51:35.6: ref_mag=14.68 +/- 0.09 new_mean_mag=14.5892 delta=0.09 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 21:58:52.13 +10:22:02.2: 14.25 +/- 0.09 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:15:12.33 +13:40:53.1: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:31:31.09 +11:18:41.8: 14.14 +/- 0.08 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:30:30.83 +12:31:19.0: 13.63 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:26:40.41 +12:56:33.6: 13.55 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:23:45.02 +09:58:01.3: 12.51 +/- 0.02 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:31:03.87 +10:22:08.5: 13.78 +/- 0.06 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:31:54.54 +16:38:37.9: 13.05 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:25:31.24 +13:30:04.4: 14.46 +/- 0.11 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:27:57.29 +11:28:03.9: 14.50 +/- 0.11 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:15:12.33 +13:40:53.1: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 21:58:52.13 +10:22:02.2: 14.09 +/- 0.07 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:31:31.09 +11:18:41.8: 14.40 +/- 0.09 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:45.02 +09:58:01.3: 12.39 +/- 0.02 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:30:30.83 +12:31:19.0: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.05
Forced photometry reference-image weighted average: 14.25 +/- 0.06
Forced photometry filter REJECTED candidate at 21:58:52.13 +10:22:02.2: ref_mag=14.15 +/- 0.05 new_mean_mag=14.3667 delta=-0.21 (need > 0.90)
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter REJECTED candidate at 22:31:31.09 +11:18:41.8: ref_mag=14.25 +/- 0.06 new_mean_mag=14.5036 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:31:54.54 +16:38:37.9: 13.13 +/- 0.03 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:26:40.41 +12:56:33.6: 13.63 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:27:57.29 +11:28:03.9: 14.57 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry filter REJECTED candidate at 22:23:45.02 +09:58:01.3: ref_mag=12.44 +/- 0.01 new_mean_mag=12.5099 delta=-0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:30:30.83 +12:31:19.0: ref_mag=13.69 +/- 0.04 new_mean_mag=13.7783 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Forced photometry reference-image weighted average: 14.54 +/- 0.08
Forced photometry filter REJECTED candidate at 22:31:54.54 +16:38:37.9: ref_mag=13.09 +/- 0.02 new_mean_mag=13.3006 delta=-0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:27:57.29 +11:28:03.9: ref_mag=14.54 +/- 0.08 new_mean_mag=14.3192 delta=0.22 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:26:40.41 +12:56:33.6: ref_mag=13.59 +/- 0.04 new_mean_mag=13.6944 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:31:03.87 +10:22:08.5: 13.71 +/- 0.06 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:25:31.24 +13:30:04.4: 14.30 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter REJECTED candidate at 22:31:03.87 +10:22:08.5: ref_mag=13.74 +/- 0.04 new_mean_mag=13.7513 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 14.36 +/- 0.07
Forced photometry filter REJECTED candidate at 22:25:31.24 +13:30:04.4: ref_mag=14.36 +/- 0.07 new_mean_mag=14.3139 delta=0.05 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:22:35.84 +16:29:22.1: 14.35 +/- 0.09 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:29:21.10 +10:22:09.5: 14.76 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:18:00.41 +11:24:00.2: 14.71 +/- 0.14 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:20:24.08 +12:58:52.3: 14.82 +/- 0.14 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:07:32.31 +12:53:51.8: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:31:02.29 +13:10:59.1: 15.01 +/- 0.18 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:24:50.70 +09:42:07.9: 14.58 +/- 0.12 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:23:44.60 +11:05:43.8: 14.68 +/- 0.14 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:31:11.14 +13:27:43.3: 14.92 +/- 0.16 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:31:02.29 +13:10:59.1: 14.77 +/- 0.12 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:31:11.14 +13:27:43.3: 14.76 +/- 0.12 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:29:21.10 +10:22:09.5: 14.65 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.10
Forced photometry filter REJECTED candidate at 22:31:02.29 +13:10:59.1: ref_mag=14.85 +/- 0.10 new_mean_mag=14.6198 delta=0.23 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:44.60 +11:05:43.8: 14.71 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.82 +/- 0.10
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:18:00.41 +11:24:00.2: 14.60 +/- 0.12 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:20:24.08 +12:58:52.3: 14.79 +/- 0.14 detection
Forced photometry filter REJECTED candidate at 22:31:11.14 +13:27:43.3: ref_mag=14.82 +/- 0.10 new_mean_mag=14.7367 delta=0.08 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:24:50.70 +09:42:07.9: 14.55 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.70 +/- 0.10
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:22:35.84 +16:29:22.1: 14.61 +/- 0.11 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:07:32.31 +12:53:51.8: 16.08 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.65 +/- 0.09
Forced photometry reference-image weighted average: 14.70 +/- 0.10
Forced photometry filter REJECTED candidate at 22:29:21.10 +10:22:09.5: ref_mag=14.70 +/- 0.10 new_mean_mag=14.5956 delta=0.11 (need > 0.90)
Forced photometry reference-image weighted average: 14.80 +/- 0.10
Forced photometry filter REJECTED candidate at 22:18:00.41 +11:24:00.2: ref_mag=14.65 +/- 0.09 new_mean_mag=14.4597 delta=0.19 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:23:44.60 +11:05:43.8: ref_mag=14.70 +/- 0.10 new_mean_mag=14.5303 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 14.57 +/- 0.08
Forced photometry filter REJECTED candidate at 22:20:24.08 +12:58:52.3: ref_mag=14.80 +/- 0.10 new_mean_mag=14.6861 delta=0.12 (need > 0.90)
Forced photometry reference-image weighted average: 14.45 +/- 0.07
Forced photometry filter REJECTED candidate at 22:22:35.84 +16:29:22.1: ref_mag=14.45 +/- 0.07 new_mean_mag=14.4447 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:24:50.70 +09:42:07.9: ref_mag=14.57 +/- 0.08 new_mean_mag=14.4508 delta=0.12 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:30:38.59 +18:10:21.1: 14.79 +/- 0.17 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:25:13.52 +15:42:55.9: 15.02 +/- 0.17 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:26:50.21 +16:55:20.9: 14.92 +/- 0.16 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:30:30.44 +11:53:51.9: 14.83 +/- 0.17 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:28:55.87 +10:38:21.2: 14.76 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:27:20.43 +09:53:39.2: 14.81 +/- 0.16 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:28:39.62 +11:48:34.3: 14.88 +/- 0.17 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:05:03.12 +10:44:05.5: 14.74 +/- 0.13 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:25:13.52 +15:42:55.9: 14.97 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:26:50.21 +16:55:20.9: 14.91 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.91 +/- 0.11
Forced photometry filter REJECTED candidate at 22:26:50.21 +16:55:20.9: ref_mag=14.91 +/- 0.11 new_mean_mag=14.7019 delta=0.21 (need > 0.90)
Forced photometry reference-image weighted average: 14.99 +/- 0.11
Forced photometry filter REJECTED candidate at 22:25:13.52 +15:42:55.9: ref_mag=14.99 +/- 0.11 new_mean_mag=14.7440 delta=0.25 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:30:38.59 +18:10:21.1: 14.88 +/- 0.17 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:30:30.44 +11:53:51.9: 14.78 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.83 +/- 0.12
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:28:39.62 +11:48:34.3: 14.85 +/- 0.15 detection
Forced photometry filter REJECTED candidate at 22:30:38.59 +18:10:21.1: ref_mag=14.83 +/- 0.12 new_mean_mag=14.6886 delta=0.15 (need > 0.90)
Forced photometry reference-image weighted average: 14.80 +/- 0.11
Forced photometry filter REJECTED candidate at 22:30:30.44 +11:53:51.9: ref_mag=14.80 +/- 0.11 new_mean_mag=14.7411 delta=0.06 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:05:03.12 +10:44:05.5: 14.63 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.11
Forced photometry filter REJECTED candidate at 22:28:39.62 +11:48:34.3: ref_mag=14.86 +/- 0.11 new_mean_mag=14.7336 delta=0.13 (need > 0.90)
Forced photometry reference-image weighted average: 14.68 +/- 0.09
Forced photometry filter REJECTED candidate at 22:05:03.12 +10:44:05.5: ref_mag=14.68 +/- 0.09 new_mean_mag=14.7038 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:27:20.43 +09:53:39.2: 14.82 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:28:55.87 +10:38:21.2: 15.04 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.82 +/- 0.11
Forced photometry reference-image weighted average: 14.88 +/- 0.11
Forced photometry filter REJECTED candidate at 22:27:20.43 +09:53:39.2: ref_mag=14.82 +/- 0.11 new_mean_mag=14.5964 delta=0.22 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:28:55.87 +10:38:21.2: ref_mag=14.88 +/- 0.11 new_mean_mag=14.5360 delta=0.34 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:29:56.32 +12:33:15.6: 15.57 +/- 0.29 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:23:07.61 +10:51:56.5: 14.92 +/- 0.16 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:30:40.19 +14:36:58.9: 14.93 +/- 0.16 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:23:55.61 +15:14:46.6: 14.70 +/- 0.16 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:28:02.31 +10:05:58.0: 14.76 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:07:09.33 +12:25:40.3: 15.04 +/- 0.17 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:09:42.78 +09:42:54.1: 14.84 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:18:39.98 +17:19:10.4: 15.16 +/- 0.18 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:29:56.32 +12:33:15.6: 15.15 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.15
Forced photometry filter REJECTED candidate at 22:29:56.32 +12:33:15.6: ref_mag=15.26 +/- 0.15 new_mean_mag=14.7998 delta=0.46 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:55.61 +15:14:46.6: 14.71 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:07.61 +10:51:56.5: 15.28 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.11
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:30:40.19 +14:36:58.9: 15.23 +/- 0.19 detection
Forced photometry filter REJECTED candidate at 22:23:55.61 +15:14:46.6: ref_mag=14.71 +/- 0.11 new_mean_mag=14.8265 delta=-0.12 (need > 0.90)
Forced photometry reference-image weighted average: 15.06 +/- 0.12
Forced photometry reference-image weighted average: 15.05 +/- 0.12
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:28:02.31 +10:05:58.0: 15.02 +/- 0.17 detection
Forced photometry filter REJECTED candidate at 22:30:40.19 +14:36:58.9: ref_mag=15.06 +/- 0.12 new_mean_mag=14.8175 delta=0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:23:07.61 +10:51:56.5: ref_mag=15.05 +/- 0.12 new_mean_mag=14.8048 delta=0.25 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:07:09.33 +12:25:40.3: 15.23 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.11
Forced photometry filter REJECTED candidate at 22:28:02.31 +10:05:58.0: ref_mag=14.87 +/- 0.11 new_mean_mag=14.7679 delta=0.10 (need > 0.90)
Forced photometry reference-image weighted average: 15.13 +/- 0.12
Forced photometry filter REJECTED candidate at 22:07:09.33 +12:25:40.3: ref_mag=15.13 +/- 0.12 new_mean_mag=14.7930 delta=0.33 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:09:42.78 +09:42:54.1: 14.91 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.87 +/- 0.10
Forced photometry filter REJECTED candidate at 22:09:42.78 +09:42:54.1: ref_mag=14.87 +/- 0.10 new_mean_mag=14.7637 delta=0.11 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:18:39.98 +17:19:10.4: 15.37 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.26 +/- 0.13
Forced photometry filter REJECTED candidate at 22:18:39.98 +17:19:10.4: ref_mag=15.26 +/- 0.13 new_mean_mag=14.8074 delta=0.45 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:27:16.79 +12:38:54.9: 15.33 +/- 0.23 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:31:06.25 +11:34:47.7: 14.96 +/- 0.17 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:22:21.79 +11:19:48.9: 15.44 +/- 0.26 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:23:05.33 +17:15:23.3: 14.95 +/- 0.17 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:27:10.68 +10:23:06.9: 15.12 +/- 0.20 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:11:44.93 +11:24:04.1: 14.95 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:23:04.76 +11:08:49.3: 15.20 +/- 0.20 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:23:25.86 +10:17:48.2: 14.94 +/- 0.17 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:27:16.79 +12:38:54.9: 15.48 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.40 +/- 0.17
Forced photometry filter REJECTED candidate at 22:27:16.79 +12:38:54.9: ref_mag=15.40 +/- 0.17 new_mean_mag=14.8698 delta=0.53 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:31:06.25 +11:34:47.7: 15.24 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.13
Forced photometry filter REJECTED candidate at 22:31:06.25 +11:34:47.7: ref_mag=15.08 +/- 0.13 new_mean_mag=14.8439 delta=0.24 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:05.33 +17:15:23.3: 15.22 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.07 +/- 0.12
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:27:10.68 +10:23:06.9: 15.44 +/- 0.25 detection
Forced photometry filter REJECTED candidate at 22:23:05.33 +17:15:23.3: ref_mag=15.07 +/- 0.12 new_mean_mag=14.8767 delta=0.19 (need > 0.90)
Forced photometry reference-image weighted average: 15.24 +/- 0.16
Forced photometry filter REJECTED candidate at 22:27:10.68 +10:23:06.9: ref_mag=15.24 +/- 0.16 new_mean_mag=14.9025 delta=0.34 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:04.76 +11:08:49.3: 15.14 +/- 0.18 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:11:44.93 +11:24:04.1: 15.01 +/- 0.14 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:25.86 +10:17:48.2: 15.07 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.17 +/- 0.13
Forced photometry filter REJECTED candidate at 22:23:04.76 +11:08:49.3: ref_mag=15.17 +/- 0.13 new_mean_mag=14.8508 delta=0.32 (need > 0.90)
Forced photometry reference-image weighted average: 14.98 +/- 0.10
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:22:21.79 +11:19:48.9: 15.03 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 22:11:44.93 +11:24:04.1: ref_mag=14.98 +/- 0.10 new_mean_mag=14.7499 delta=0.23 (need > 0.90)
Forced photometry reference-image weighted average: 15.14 +/- 0.14
Forced photometry reference-image weighted average: 15.00 +/- 0.12
Forced photometry filter REJECTED candidate at 22:22:21.79 +11:19:48.9: ref_mag=15.14 +/- 0.14 new_mean_mag=14.7931 delta=0.35 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:23:25.86 +10:17:48.2: ref_mag=15.00 +/- 0.12 new_mean_mag=14.7197 delta=0.28 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:26:36.52 +14:09:42.3: 15.03 +/- 0.17 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:26:32.11 +12:51:04.2: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:04:31.49 +10:31:34.9: 15.51 +/- 0.26 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:15:54.04 +12:03:41.1: 15.22 +/- 0.18 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 21:59:01.47 +15:17:48.5: 14.72 +/- 0.14 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:26:36.52 +14:09:42.3: 15.08 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.06 +/- 0.12
Forced photometry filter REJECTED candidate at 22:26:36.52 +14:09:42.3: ref_mag=15.06 +/- 0.12 new_mean_mag=14.8082 delta=0.25 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:26:32.11 +12:51:04.2: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:04:31.49 +10:31:34.9: 14.96 +/- 0.14 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:15:54.04 +12:03:41.1: 14.94 +/- 0.13 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.13
Forced photometry filter REJECTED candidate at 22:04:31.49 +10:31:34.9: ref_mag=15.08 +/- 0.13 new_mean_mag=14.8756 delta=0.20 (need > 0.90)
Forced photometry reference-image weighted average: 15.04 +/- 0.11
Forced photometry filter REJECTED candidate at 22:15:54.04 +12:03:41.1: ref_mag=15.04 +/- 0.11 new_mean_mag=14.8294 delta=0.21 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 21:59:01.47 +15:17:48.5: 14.56 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.08
Forced photometry filter REJECTED candidate at 21:59:01.47 +15:17:48.5: ref_mag=14.62 +/- 0.08 new_mean_mag=14.7596 delta=-0.14 (need > 0.90)
Adding exclusion_list_local.txt__out94042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94704.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 93938_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 93938_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 93939_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 93939_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 93947_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 93947_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 93951_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 93951_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 93953_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 93953_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 93955_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 93955_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 93957_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 93957_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 93970_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 93970_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 93975_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 93975_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 93980_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 93980_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 93983_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 93983_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 93985_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 93985_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94004_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94004_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94041_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94041_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94042_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
Preparing report for the candidate 94042_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
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Considering the candidate 94076_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94076_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94116_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94116_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94126_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94126_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94216_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94216_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94220_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94220_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94246_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
Preparing report for the candidate 94246_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
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Considering the candidate 94249_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94249_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94276_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94276_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94307_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94307_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94312_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94312_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94349_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94349_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94389_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94389_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94401_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94401_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94413_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94413_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94421_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94421_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94451_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94451_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94455_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94455_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94456_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94456_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94464_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94464_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94501_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94501_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94508_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94508_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94515_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94515_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94530_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94530_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94536_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94536_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94563_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94563_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94586_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94586_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94589_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94589_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94592_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94592_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94597_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94597_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94603_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94603_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94629_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94629_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94643_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94643_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94645_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94645_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94654_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94654_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94670_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94670_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94673_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94673_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94684_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94684_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94687_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94687_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94692_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94692_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94704_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
Preparing report for the candidate 94704_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
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Considering the candidate 94733_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94733_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94751_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94751_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 94856_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 94856_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
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Considering the candidate 30496_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 30496_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
**** FOUND 22:03:33.95 +14:00:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21757_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
Preparing report for the candidate 21757_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
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Considering the candidate 15050_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415
The candidate 15050_fd_Peg-09-Q2b1x1_2026-08-19_04-05-50_20.00sec_-0.00C_LIGHT_0415 did not pass the final checks
