This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs
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,2461269.8672,10.12,0.05,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 20260817.3672 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3672 2461269.8672 12.68 22:16:23.00 +13:57:12.3
75.57851 -34.29995 galactic Peg Second-epoch detections are separated by 0.7" and 8.9 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 22:16:23.00 +13:57:12.3: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:16:23.00 +13:57:12.3: 16.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461269.8672,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260817.3672 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3672 2461269.8672 14.22 22:08:57.09 +13:02:25.1
73.23671 -33.72564 galactic Peg Second-epoch detections are separated by 1.0" and 9.0 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 -0 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 22:08:57.09 +13:02:25.1: 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 22:08:57.09 +13:02:25.1: 16.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461269.8672,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260817.3672 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 17.3672 2461269.8672 11.29 22:12:16.25 +14:33:11.0
75.18576 -33.18376 galactic Peg Second-epoch detections are separated by 0.3" and 8.8 pix
The object was found in VSX 2" RS Peg
Type: M
# Max. Min./Amp. JD0 Period
8.200 V 14.700 V 2445161.00000 415.400000000000 M6e-M9e
The object was not found in astcheck.
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:12:16.25 +14:33:11.0: 12.42 +/- 0.02 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:12:16.25 +14:33:11.0: 12.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
RS Peg,2461269.8672,11.29,0.05,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
RS Peg 20260817.3672 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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,2461269.8672,10.12,0.05,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 20260817.3672 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461269.86756931 17.08.2026 08:49:07.988 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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: 4 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): 9218
Objects passed selection criteria: 9213
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: 8936.25
Average stars matched: 7958 (89.053 %)
Memory usage VmPeak: 236100 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 17 04:12:44 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: 2461269.86756931 17.08.2026 08:49:07.988 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 69
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: 22 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): 54098
Objects passed selection criteria: 53981
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: 53595.2
Average stars matched: 48206.5 (89.9455 %)
Memory usage VmPeak: 285060 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 17 04:13:45 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_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461269.86687872
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_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits exists and is non-empty
wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits (1st new image)
verification OK: wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.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: 22:13:20.178 +13:59:52.50 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 22:13:20.178 +13:59:52.50
Angular distance between the image centers 0.0226 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits (2nd new image)
verification OK: wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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: 22:13:22.977 +13:59:19.35 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 22:13:22.977 +13:59:19.35
Angular distance between the image centers 0.0265 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 22:13:20.178 +13:59:52.50
Second-epoch second image center 22:13:22.977 +13:59:19.35
Angular distance between the image centers 0.01459 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.6b35MgGRg6
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.tduKSChawJ
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_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits &> /tmp/tmp.stpVMCuvGk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits &> /tmp/tmp.Ap2w4OCxHH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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
2.7 pix fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
2.7 pix fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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
15.1 mag. fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
15.1 mag. fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
All-image limiting magnitude estimate: 15.1 (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.6b35MgGRg6 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/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.tduKSChawJ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/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.stpVMCuvGk (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
Checking if the catalog wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.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_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
WCS catalog name: wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.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=695, bad_region=2664, passed=12171
Got 12171 stars (including 9055 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits.wcscat
util/solve_plate_with_UCAC5 got 12171 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 19.3)
Done reading UCAC5 zone files...
Matched 4699 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4673 matched stars entering correct_measured_positions(), 4673 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4673 matched stars entering correct_measured_positions(), 10083 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 4699 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4673 matched stars entering correct_measured_positions(), 10083 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4673 matched stars entering correct_measured_positions(), 10083 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4673 stars left (next iteration limit 5140)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4673 robust_rms=6.781 arcsec worst_quadrant_rms=8.497 arcsec
SIP_REFIT: SIP order 3 trial: matched=4673 robust_rms=0.365 arcsec worst_quadrant_rms=0.394 arcsec
SIP_REFIT: SIP order 5 trial: matched=4673 robust_rms=0.338 arcsec worst_quadrant_rms=0.396 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4673 robust_rms_before=0.650 arcsec robust_rms_before_corrected=0.351 arcsec robust_rms_after=0.365 arcsec worst_quadrant_rms_before=0.415 worst_quadrant_rms_after=0.394
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.415 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits N_match=4673 sigma_overall_arcsec=0.354 sigma_q1_arcsec=0.313 sigma_q2_arcsec=0.394 sigma_q3_arcsec=0.353 sigma_q4_arcsec=0.399 n_q1=1562 n_q2=969 n_q3=1322 n_q4=820 worst_quadrant_to_overall_ratio=1.128
The image catalog is written to wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits -region wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.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.Ap2w4OCxHH (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
Checking if the catalog wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
WCS catalog name: wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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=744, bad_region=2687, passed=12109
Got 12109 stars (including 8945 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits.wcscat
util/solve_plate_with_UCAC5 got 12109 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 19.3)
Done reading UCAC5 zone files...
Matched 4698 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4671 matched stars entering correct_measured_positions(), 4671 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4671 matched stars entering correct_measured_positions(), 10023 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 4697 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4671 matched stars entering correct_measured_positions(), 10023 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4671 matched stars entering correct_measured_positions(), 10023 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4671 stars left (next iteration limit 5138)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4671 robust_rms=6.856 arcsec worst_quadrant_rms=8.235 arcsec
SIP_REFIT: SIP order 3 trial: matched=4671 robust_rms=0.377 arcsec worst_quadrant_rms=0.413 arcsec
SIP_REFIT: SIP order 5 trial: matched=4671 robust_rms=0.343 arcsec worst_quadrant_rms=0.394 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4671 robust_rms_before=0.677 arcsec robust_rms_before_corrected=0.354 arcsec robust_rms_after=0.377 arcsec worst_quadrant_rms_before=0.418 worst_quadrant_rms_after=0.413
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.418 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits N_match=4671 sigma_overall_arcsec=0.362 sigma_q1_arcsec=0.309 sigma_q2_arcsec=0.408 sigma_q3_arcsec=0.349 sigma_q4_arcsec=0.433 n_q1=1552 n_q2=984 n_q3=1317 n_q4=818 worst_quadrant_to_overall_ratio=1.195
The image catalog is written to wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits -region wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits to local_wcs_cache/
'wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits' -> 'local_wcs_cache/wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits'
Saving the final (post-refit) wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits to local_wcs_cache/
'wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits' -> 'local_wcs_cache/wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits sigma_overall=0.354 worst_q_ratio=1.128
new2=fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits sigma_overall=0.362 worst_q_ratio=1.195
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_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410_astrometric_residuals.png (4673 matched stars from wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411_astrometric_residuals.png (4671 matched stars from wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits'
Saving fully-calibrated image wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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 22:28:32.85 +16:07:23.4: 10.89 +/- 0.00 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:16:35.42 +14:45:04.9: 12.15 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:14:35.11 +16:41:40.5: 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 22:10:35.43 +13:34:20.8: 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 22:12:16.22 +14:33:11.0: 12.17 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:12:19.95 +13:23:44.9: 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 22:11:08.82 +14:59:43.6: 12.16 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:10:35.43 +13:34:20.8: 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 22:28:32.85 +16:07:23.4: 10.84 +/- 0.00 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:12:16.22 +14:33:11.0: 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 +13:23:44.9: 12.26 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:16:35.42 +14:45:04.9: 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 +14:59:43.6: 12.22 +/- 0.01 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:14:35.11 +16:41:40.5: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.86 +/- 0.00
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter REJECTED candidate at 22:28:32.85 +16:07:23.4: ref_mag=10.86 +/- 0.00 new_mean_mag=11.1464 delta=-0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:10:35.43 +13:34:20.8: ref_mag=12.04 +/- 0.01 new_mean_mag=12.0470 delta=-0.00 (need > 0.90)
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry filter REJECTED candidate at 22:11:08.82 +14:59:43.6: ref_mag=12.19 +/- 0.01 new_mean_mag=12.1839 delta=0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:12:19.95 +13:23:44.9: ref_mag=12.24 +/- 0.01 new_mean_mag=12.2434 delta=0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:16:35.42 +14:45:04.9: ref_mag=12.14 +/- 0.01 new_mean_mag=12.1117 delta=0.03 (need > 0.90)
Forced photometry filter KEPT candidate at 22:12:16.22 +14:33:11.0: ref_mag=12.09 +/- 0.01 new_mean_mag=11.1515 delta=0.94 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:14:35.11 +16:41:40.5: ref_mag=12.15 +/- 0.01 new_mean_mag=12.1687 delta=-0.02 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out05715.dat to exclusion_list_gaiadr2.txt
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
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Considering the candidate 22641_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 22641_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 22646_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 22646_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
**** FOUND 22:03:33.97 +14:00:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22652_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 22652_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 22653_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 22653_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 22654_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 22654_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 22655_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 22655_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 22657_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 22657_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 05715_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 05715_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
**** FOUND 22:12:16.22 +14:33:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 1.346 2735144236198245376 333.06747997741 +14.55341585394 8.3831 6.8722 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21208_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 21208_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
**** FOUND 22:11:37.48 +14:21:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03891_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
Preparing report for the candidate 03891_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
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_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits exists and is non-empty
wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits (1st new image)
verification OK: wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.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: 22:13:20.178 +13:59:52.50 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 22:13:20.178 +13:59:52.50
Angular distance between the image centers 0.0226 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits (2nd new image)
verification OK: wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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: 22:13:22.977 +13:59:19.35 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 22:13:22.977 +13:59:19.35
Angular distance between the image centers 0.0265 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 22:13:20.178 +13:59:52.50
Second-epoch second image center 22:13:22.977 +13:59:19.35
Angular distance between the image centers 0.01459 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.CrNsi7ObmO
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.1z4QZOUrX9
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_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits &> /tmp/tmp.WK2F3lkswa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits &> /tmp/tmp.zwLPGUGV5j
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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 44 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
2.5 pix fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
2.5 pix fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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
15.2 mag. fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
15.2 mag. fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.5 (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.CrNsi7ObmO (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/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.1z4QZOUrX9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/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.WK2F3lkswa (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
Checking if the catalog wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.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_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
WCS catalog name: wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.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=11, blended=5184, bad_region=10853, passed=61640
Got 61640 stars (including 47867 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits.wcscat
util/solve_plate_with_UCAC5 got 61640 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 19.3)
Done reading UCAC5 zone files...
Matched 4685 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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4664 matched stars entering correct_measured_positions(), 53349 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 19.3)
Done reading UCAC5 zone files...
Matched 4685 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4663 matched stars entering correct_measured_positions(), 53349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4663 matched stars entering correct_measured_positions(), 53350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4663 stars left (next iteration limit 5130)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.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=4663 robust_rms=6.669 arcsec worst_quadrant_rms=9.185 arcsec
SIP_REFIT: SIP order 3 trial: matched=4663 robust_rms=0.365 arcsec worst_quadrant_rms=0.394 arcsec
SIP_REFIT: SIP order 5 trial: matched=4663 robust_rms=0.337 arcsec worst_quadrant_rms=0.392 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4663 robust_rms_before=0.656 arcsec robust_rms_before_corrected=0.348 arcsec robust_rms_after=0.365 arcsec worst_quadrant_rms_before=0.411 worst_quadrant_rms_after=0.394
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.411 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits N_match=4663 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.316 sigma_q2_arcsec=0.387 sigma_q3_arcsec=0.336 sigma_q4_arcsec=0.413 n_q1=1594 n_q2=919 n_q3=1359 n_q4=791 worst_quadrant_to_overall_ratio=1.180
The image catalog is written to wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits -region wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.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.zwLPGUGV5j (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
Checking if the catalog wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits.wcscat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
WCS catalog name: wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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=15, blended=5186, bad_region=10873, passed=61682
Got 61682 stars (including 47921 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits.wcscat
util/solve_plate_with_UCAC5 got 61682 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 19.3)
Done reading UCAC5 zone files...
Matched 4685 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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4664 matched stars entering correct_measured_positions(), 53427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 4684 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(), 53427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4664 matched stars entering correct_measured_positions(), 53427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4664 stars left (next iteration limit 5130)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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=4664 robust_rms=6.814 arcsec worst_quadrant_rms=9.062 arcsec
SIP_REFIT: SIP order 3 trial: matched=4664 robust_rms=0.373 arcsec worst_quadrant_rms=0.409 arcsec
SIP_REFIT: SIP order 5 trial: matched=4664 robust_rms=0.341 arcsec worst_quadrant_rms=0.392 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4664 robust_rms_before=0.678 arcsec robust_rms_before_corrected=0.353 arcsec robust_rms_after=0.373 arcsec worst_quadrant_rms_before=0.413 worst_quadrant_rms_after=0.409
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.413 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits N_match=4664 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.315 sigma_q2_arcsec=0.413 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.422 n_q1=1592 n_q2=923 n_q3=1355 n_q4=794 worst_quadrant_to_overall_ratio=1.172
The image catalog is written to wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits -region wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-48-08_20.00sec_-0.00C_LIGHT_0410.fits
Saving fully-calibrated image wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-17_CI_Peg-09-Q2b1x1_041036_TTUQ2b1x1_3954546_9lvMuWjs/wcs_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411.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 22:04:20.41 +12:19:03.6: 14.46 +/- 0.10 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:20:58.01 +17:40:45.6: 14.38 +/- 0.10 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:23:36.96 +11:51:39.4: 14.63 +/- 0.13 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:23:45.02 +09:58:01.0: 12.52 +/- 0.02 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:27:42.09 +12:01:17.1: 13.81 +/- 0.06 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:26:29.93 +10:55:16.1: 14.86 +/- 0.16 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:23:56.49 +11:31:06.6: 14.60 +/- 0.12 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:16:23.00 +13:57:12.3: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 21:55:29.22 +10:40:26.8: 14.26 +/- 0.09 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:05:10.68 +14:17:51.3: 14.50 +/- 0.10 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:20:58.01 +17:40:45.6: 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 22:04:20.41 +12:19:03.6: 14.45 +/- 0.09 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:56.49 +11:31:06.6: 14.63 +/- 0.11 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:36.96 +11:51:39.4: 14.73 +/- 0.13 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 21:55:29.22 +10:40:26.8: 14.18 +/- 0.07 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:27:42.09 +12:01:17.1: 13.81 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:16:23.00 +13:57:12.3: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:05:10.68 +14:17:51.3: 14.54 +/- 0.10 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:26:29.93 +10:55:16.1: 14.82 +/- 0.14 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:45.02 +09:58:01.0: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.06
Forced photometry reference-image weighted average: 14.45 +/- 0.06
Forced photometry reference-image weighted average: 14.22 +/- 0.06
Forced photometry filter REJECTED candidate at 22:20:58.01 +17:40:45.6: ref_mag=14.34 +/- 0.06 new_mean_mag=14.5808 delta=-0.24 (need > 0.90)
Forced photometry reference-image weighted average: 14.69 +/- 0.09
Forced photometry filter REJECTED candidate at 22:04:20.41 +12:19:03.6: ref_mag=14.45 +/- 0.06 new_mean_mag=14.2704 delta=0.18 (need > 0.90)
Forced photometry reference-image weighted average: 14.84 +/- 0.10
Forced photometry reference-image weighted average: 14.62 +/- 0.08
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry reference-image weighted average: 14.52 +/- 0.07
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry filter REJECTED candidate at 21:55:29.22 +10:40:26.8: ref_mag=14.22 +/- 0.06 new_mean_mag=14.6483 delta=-0.43 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:23:36.96 +11:51:39.4: ref_mag=14.69 +/- 0.09 new_mean_mag=14.7357 delta=-0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:26:29.93 +10:55:16.1: ref_mag=14.84 +/- 0.10 new_mean_mag=14.6012 delta=0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:27:42.09 +12:01:17.1: ref_mag=13.81 +/- 0.04 new_mean_mag=14.0857 delta=-0.27 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:23:56.49 +11:31:06.6: ref_mag=14.62 +/- 0.08 new_mean_mag=14.5321 delta=0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:05:10.68 +14:17:51.3: ref_mag=14.52 +/- 0.07 new_mean_mag=14.6746 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:23:45.02 +09:58:01.0: ref_mag=12.44 +/- 0.01 new_mean_mag=12.5298 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 22:31:03.86 +10:22:08.9: 13.77 +/- 0.06 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:29:14.84 +10:32:40.7: 15.40 +/- 0.27 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:10:12.15 +12:24:56.3: 14.02 +/- 0.08 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:08:57.09 +13:02:25.1: 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 22:27:20.48 +09:53:38.0: 14.87 +/- 0.17 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:28:39.68 +11:48:33.7: 14.88 +/- 0.16 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:25:31.08 +13:30:05.1: 14.44 +/- 0.10 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:30:30.73 +12:31:18.6: 13.68 +/- 0.05 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:28:55.88 +10:38:22.1: 14.77 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:30:30.73 +12:31:18.6: 13.79 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:31:03.86 +10:22:08.9: 13.70 +/- 0.05 detection
Forced photometry filter REJECTED candidate at 22:30:30.73 +12:31:18.6: ref_mag=13.73 +/- 0.04 new_mean_mag=13.7565 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:10:12.15 +12:24:56.3: 14.01 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:27:20.48 +09:53:38.0: 14.85 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:29:14.84 +10:32:40.7: 15.48 +/- 0.27 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:25:31.08 +13:30:05.1: 14.22 +/- 0.08 detection
Forced photometry filter REJECTED candidate at 22:31:03.86 +10:22:08.9: ref_mag=13.73 +/- 0.04 new_mean_mag=13.6930 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.01 +/- 0.05
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:28:39.68 +11:48:33.7: 14.87 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:08:57.09 +13:02:25.1: 16.06 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 22:10:12.15 +12:24:56.3: ref_mag=14.01 +/- 0.05 new_mean_mag=13.9353 delta=0.08 (need > 0.90)
Forced photometry reference-image weighted average: 15.44 +/- 0.19
Forced photometry reference-image weighted average: 14.30 +/- 0.06
Forced photometry reference-image weighted average: 14.86 +/- 0.11
Forced photometry filter REJECTED candidate at 22:29:14.84 +10:32:40.7: ref_mag=15.44 +/- 0.19 new_mean_mag=14.7681 delta=0.68 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:27:20.48 +09:53:38.0: ref_mag=14.86 +/- 0.11 new_mean_mag=14.5175 delta=0.34 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:25:31.08 +13:30:05.1: ref_mag=14.30 +/- 0.06 new_mean_mag=14.2976 delta=0.00 (need > 0.90)
Forced photometry reference-image weighted average: 14.88 +/- 0.11
Forced photometry filter REJECTED candidate at 22:28:39.68 +11:48:33.7: ref_mag=14.88 +/- 0.11 new_mean_mag=14.6383 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 22:28:55.88 +10:38:22.1: 15.03 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.11
Forced photometry filter REJECTED candidate at 22:28:55.88 +10:38:22.1: ref_mag=14.88 +/- 0.11 new_mean_mag=14.5789 delta=0.30 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:27:57.29 +11:28:03.8: 14.51 +/- 0.11 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:29:21.19 +10:22:09.3: 14.77 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:25:13.53 +15:42:56.1: 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 22:26:42.06 +10:57:55.4: 15.40 +/- 0.25 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:29:02.26 +12:27:43.1: 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 22:23:55.62 +15:14:47.0: 14.69 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:23:44.68 +11:05:44.6: 14.67 +/- 0.14 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:25:14.69 +10:36:55.6: 14.89 +/- 0.16 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:27:57.29 +11:28:03.8: 14.56 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.54 +/- 0.08
Forced photometry filter REJECTED candidate at 22:27:57.29 +11:28:03.8: ref_mag=14.54 +/- 0.08 new_mean_mag=14.5050 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 22:25:13.53 +15:42:56.1: 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 22:29:02.26 +12:27:43.1: 15.13 +/- 0.18 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:29:21.19 +10:22:09.3: 14.63 +/- 0.13 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:26:42.06 +10:57:55.4: 15.33 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.11
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:55.62 +15:14:47.0: 14.71 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.12
Forced photometry reference-image weighted average: 14.69 +/- 0.10
Forced photometry filter REJECTED candidate at 22:25:13.53 +15:42:56.1: ref_mag=14.99 +/- 0.11 new_mean_mag=14.7045 delta=0.29 (need > 0.90)
Forced photometry reference-image weighted average: 15.36 +/- 0.16
Forced photometry filter REJECTED candidate at 22:29:02.26 +12:27:43.1: ref_mag=15.04 +/- 0.12 new_mean_mag=14.7456 delta=0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:29:21.19 +10:22:09.3: ref_mag=14.69 +/- 0.10 new_mean_mag=14.7212 delta=-0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:26:42.06 +10:57:55.4: ref_mag=15.36 +/- 0.16 new_mean_mag=14.7897 delta=0.57 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:44.68 +11:05:44.6: 14.71 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.70 +/- 0.11
Forced photometry filter REJECTED candidate at 22:23:55.62 +15:14:47.0: ref_mag=14.70 +/- 0.11 new_mean_mag=14.6568 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.69 +/- 0.09
Forced photometry filter REJECTED candidate at 22:23:44.68 +11:05:44.6: ref_mag=14.69 +/- 0.09 new_mean_mag=14.5614 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 22:25:14.69 +10:36:55.6: 14.73 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.10
Forced photometry filter REJECTED candidate at 22:25:14.69 +10:36:55.6: ref_mag=14.79 +/- 0.10 new_mean_mag=14.7706 delta=0.02 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:23:04.55 +10:14:21.7: 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 22:30:30.42 +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 22:26:12.20 +12:52:28.1: 14.72 +/- 0.13 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:26:33.28 +14:20:29.1: 14.95 +/- 0.16 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:22:21.85 +11:19:48.6: 15.48 +/- 0.27 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 21:59:03.75 +13:24:48.7: 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 22:29:23.53 +13:34:22.6: 15.65 +/- 0.31 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:25:13.80 +10:42:50.3: 15.26 +/- 0.22 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:23:04.55 +10:14:21.7: 15.01 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.13
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:29:23.53 +13:34:22.6: 15.65 +/- 0.27 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:26:33.28 +14:20:29.1: 14.92 +/- 0.13 detection
Forced photometry filter REJECTED candidate at 22:23:04.55 +10:14:21.7: ref_mag=15.05 +/- 0.13 new_mean_mag=14.6441 delta=0.41 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:22:21.85 +11:19:48.6: 15.06 +/- 0.16 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:30:30.42 +11:53:51.9: 14.77 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:26:12.20 +12:52:28.1: 14.43 +/- 0.09 detection
Forced photometry reference-image weighted average: 15.65 +/- 0.21
Forced photometry reference-image weighted average: 14.93 +/- 0.10
Forced photometry filter KEPT candidate at 22:29:23.53 +13:34:22.6: ref_mag=15.65 +/- 0.21 new_mean_mag=14.7281 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 15.18 +/- 0.14
Forced photometry filter REJECTED candidate at 22:26:33.28 +14:20:29.1: ref_mag=14.93 +/- 0.10 new_mean_mag=14.7303 delta=0.20 (need > 0.90)
Forced photometry reference-image weighted average: 14.80 +/- 0.11
Forced photometry reference-image weighted average: 14.53 +/- 0.07
Forced photometry filter REJECTED candidate at 22:22:21.85 +11:19:48.6: ref_mag=15.18 +/- 0.14 new_mean_mag=14.7196 delta=0.46 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:30:30.42 +11:53:51.9: ref_mag=14.80 +/- 0.11 new_mean_mag=14.6865 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 21:59:03.75 +13:24:48.7: 14.71 +/- 0.12 detection
Forced photometry filter REJECTED candidate at 22:26:12.20 +12:52:28.1: ref_mag=14.53 +/- 0.07 new_mean_mag=14.6502 delta=-0.12 (need > 0.90)
Forced photometry reference-image weighted average: 14.76 +/- 0.09
Forced photometry filter REJECTED candidate at 21:59:03.75 +13:24:48.7: ref_mag=14.76 +/- 0.09 new_mean_mag=14.7039 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 22:25:13.80 +10:42:50.3: 15.23 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.24 +/- 0.15
Forced photometry filter REJECTED candidate at 22:25:13.80 +10:42:50.3: ref_mag=15.24 +/- 0.15 new_mean_mag=14.8372 delta=0.41 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:21:14.09 +10:52:19.0: 14.96 +/- 0.18 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:22:19.97 +12:01:08.7: 15.21 +/- 0.21 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:04:31.50 +10:31:35.0: 15.51 +/- 0.27 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 21:57:40.64 +12:21:00.5: 14.98 +/- 0.17 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 21:56:34.79 +13:16:39.2: 15.03 +/- 0.17 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:21:14.09 +10:52:19.0: 15.11 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.13
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:22:19.97 +12:01:08.7: 15.44 +/- 0.23 detection
Forced photometry filter REJECTED candidate at 22:21:14.09 +10:52:19.0: ref_mag=15.03 +/- 0.13 new_mean_mag=14.8345 delta=0.20 (need > 0.90)
Forced photometry reference-image weighted average: 15.31 +/- 0.15
Forced photometry filter REJECTED candidate at 22:22:19.97 +12:01:08.7: ref_mag=15.31 +/- 0.15 new_mean_mag=14.8492 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 21:57:40.64 +12:21:00.5: 15.03 +/- 0.15 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:04:31.50 +10:31:35.0: 14.95 +/- 0.14 detection
Forced photometry on wcs_Peg-09-Q2b1x1_2026-06-17_03-34-27_20.00sec_5.00C_LIGHT_0368.fits at 22:12:16.25 +14:33:11.0: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.11
Forced photometry filter REJECTED candidate at 21:57:40.64 +12:21:00.5: ref_mag=15.01 +/- 0.11 new_mean_mag=14.8415 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 15.08 +/- 0.13
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 21:56:34.79 +13:16:39.2: 15.19 +/- 0.17 detection
Forced photometry filter REJECTED candidate at 22:04:31.50 +10:31:35.0: ref_mag=15.08 +/- 0.13 new_mean_mag=14.7851 delta=0.29 (need > 0.90)
Forced photometry reference-image weighted average: 15.11 +/- 0.12
Forced photometry filter REJECTED candidate at 21:56:34.79 +13:16:39.2: ref_mag=15.11 +/- 0.12 new_mean_mag=14.8896 delta=0.22 (need > 0.90)
Forced photometry on wcs_Peg-09-Q2b1x1_2026-07-20_05-09-57_20.00sec_5.00C_LIGHT_0471.fits at 22:12:16.25 +14:33:11.0: 12.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry filter KEPT candidate at 22:12:16.25 +14:33:11.0: ref_mag=12.37 +/- 0.01 new_mean_mag=11.2903 delta=1.08 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out94726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out33488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94217.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 93887_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 93887_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 93901_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 93901_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 93908_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 93908_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 93917_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 93917_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 93922_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 93922_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 93942_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 93942_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 93951_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 93951_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 93963_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 93963_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 93990_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 93990_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 93999_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
Preparing report for the candidate 93999_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
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Considering the candidate 94074_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94074_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
**** FOUND 22:19:51.82 +16:51:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94082_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94082_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94092_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94092_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94137_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94137_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94206_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94206_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94217_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
Preparing report for the candidate 94217_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
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Considering the candidate 94322_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94322_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94388_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94388_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94468_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94468_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94474_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94474_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94483_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94483_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94514_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94514_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94518_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94518_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94522_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94522_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94532_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94532_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94575_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94575_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94585_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94585_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94593_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94593_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94597_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94597_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94603_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94603_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94636_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94636_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94640_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94640_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94682_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94682_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94726_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94726_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
**** FOUND 22:29:23.53 +13:34:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 0.416 2731313812564599808 337.34811141914 +13.57285093474 15.3491 14.9095 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 94753_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94753_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94770_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94770_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94793_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94793_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94815_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94815_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 94856_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 94856_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 95134_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 95134_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 95137_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 95137_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
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Considering the candidate 30496_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411
The candidate 30496_fd_Peg-09-Q2b1x1_2026-08-17_03-49-07_20.00sec_0.00C_LIGHT_0411 did not pass the final checks
