This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 10 28.2032 2461341.7032 13.60 22:44:17.41 +11:56:13.8
80.47582 -40.22769 galactic Peg Second-epoch detections are separated by 2.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.170 Maria -1 -1 1 13.5 -0 -0
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:44:17.41 +11:56:13.8: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:44:17.41 +11:56:13.8: 15.80 +/- 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,2461341.7032,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261028.2032 13.60CV 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 10 28.2032 2461341.7032 13.60 22:47:07.56 +10:48:04.7
80.27907 -41.55099 galactic Peg Second-epoch detections are separated by 0.2" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.978 Aidamina -1 -0 1 13.7 -0 0
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:47:07.56 +10:48:04.7: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:47:07.56 +10:48:04.7: 15.85 +/- 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,2461341.7032,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261028.2032 13.60CV 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 10 28.2032 2461341.7032 14.01 23:16:51.23 +15:34:03.3
91.86086 -41.52773 galactic Peg Second-epoch detections are separated by 2.2" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.665 Sabine 0 -1 1 13.9 -0 -0
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:16:51.23 +15:34:03.3: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:16:51.23 +15:34:03.3: 16.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461341.7032,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261028.2032 14.01CV 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 10 28.2032 2461341.7032 14.46 23:27:42.71 +18:05:13.3
96.43275 -40.43727 galactic Peg Second-epoch detections are separated by 2.2" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1468 Zomba -0 0 0 14.5 0 0
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:27:42.71 +18:05:13.3: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:27:42.71 +18:05:13.3: 15.90 +/- 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,2461341.7032,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261028.2032 14.46CV 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 10 28.2032 2461341.7032 14.51 22:55:06.64 +16:53:29.2
86.92168 -37.71527 galactic Peg Second-epoch detections are separated by 1.5" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.879 Ricarda -1 0 1 14.4 -0 -0
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:55:06.64 +16:53:29.2: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:55:06.64 +16:53:29.2: 15.93 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461341.7032,14.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261028.2032 14.51CV 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: 2461242.89976286 21.07.2026 09:35:29.511 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
First image: 2461242.89976286 21.07.2026 09:35:29.511 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Last image: 2461341.70347909 28.10.2026 04:52:50.593 /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.17
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: 3 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): 8730
Objects passed selection criteria: 8708
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 7246.5
Average stars matched: 7110.5 (98.1232 %)
Memory usage VmPeak: 234940 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Oct 27 23:58:42 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: 2461242.89976286 21.07.2026 09:35:29.511 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
First image: 2461242.89976286 21.07.2026 09:35:29.511 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Last image: 2461341.70347909 28.10.2026 04:52:50.593 /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 45
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -6.92
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: 16 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): 49100
Objects passed selection criteria: 48981
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 43703.8
Average stars matched: 42529 (97.312 %)
Memory usage VmPeak: 270544 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Oct 27 23:59:50 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
SExtractor catalog cache: saved Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.cat to cache
SExtractor catalog cache: saved Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461341.70284278
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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits exists and is non-empty
wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits exists and is non-empty
wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits exists and is non-empty
wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits (1st reference image)
verification OK: wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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: 23:06:39.243 +14:00:09.40 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-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits (1st new image)
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:07:03.581 +13:59:16.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:06:39.243 +14:00:09.40
Second-epoch image center 23:07:03.581 +13:59:16.73
Angular distance between the image centers 0.0995 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits (2nd new image)
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:07:01.283 +13:59:50.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:06:39.243 +14:00:09.40
Second-epoch image center 23:07:01.283 +13:59:50.16
Angular distance between the image centers 0.0893 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 23:07:03.581 +13:59:16.73
Second-epoch second image center 23:07:01.283 +13:59:50.16
Angular distance between the image centers 0.01314 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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits &> /tmp/tmp.nxlEMUkOIo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits &> /tmp/tmp.vk7PquF2bQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits &> /tmp/tmp.6uvZF306XE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits &> /tmp/tmp.TD2aUjvd7v
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits and wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits and wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
Found non-empty wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits and wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
The reference image (wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits) and catalog (wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat) found
'wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat' -> 'wcsmag.cat'
Read 9326 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4001 to 354.8631 deg, Dec +8.6411 to +19.2659 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 338.4001 to 354.8631 deg, Dec 8.6411 to 19.2659 deg
Loaded 5954 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): 4864 out of 5041 total matches.
Matched with Tycho-2 5041 out of 9326 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.690300
a=0.000000 b=1.000000 c=22.690300
From vast_summary.log: estimated ref. image limiting mag.: -7.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9326 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4001 to 354.8631 deg, Dec +8.6411 to +19.2659 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 338.4001 to 354.8631 deg, Dec 8.6411 to 19.2659 deg
Loaded 5954 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): 4864 out of 5041 total matches.
Matched with Tycho-2 5041 out of 9326 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Forced-photometry filter: calibrated wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits -> calib.txt_param_ref_wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits (aperture=6.3)
Read 8960 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4002 to 354.8630 deg, Dec +8.6412 to +19.2650 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 338.4002 to 354.8630 deg, Dec 8.6412 to 19.2650 deg
Loaded 5954 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): 4852 out of 5019 total matches.
Matched with Tycho-2 5019 out of 8960 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
Forced-photometry filter: calibrated wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits -> calib.txt_param_ref_wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
2.2 pix Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
2.2 pix fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
2.2 pix fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
Limiting magnitude estimates:
15.5 mag. Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
15.5 mag. Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
14.9 mag. fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
14.9 mag. fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 11.7 (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.nxlEMUkOIo (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits' -> 'wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
WCS-calibrated image found: wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Checking if the catalog wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
WCS catalog name: wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=501, bad_region=0, passed=9326
Got 9326 stars (including 8810 good ones) from the SExtractor catalog wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
util/solve_plate_with_UCAC5 got 9326 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 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 4869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 9326 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 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 9326 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 9326 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4869 stars left (next iteration limit 5355)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits N_match=4869 sigma_overall_arcsec=0.391 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.406 sigma_q4_arcsec=0.404 n_q1=1230 n_q2=1155 n_q3=1368 n_q4=1116 worst_quadrant_to_overall_ratio=1.097
WCS_HEADER_DIAG: file=Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits selection=current_pairs N_selected=4869 N_valid=4869 bias_ra_arcsec=0.010 bias_dec_arcsec=0.001 median_sep_arcsec=0.298 p95_sep_arcsec=1.296 n_q1=1230 n_q2=1155 n_q3=1368 n_q4=1116 occupied_cells_4x4=16/16
The image catalog is written to wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits -region wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.vk7PquF2bQ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.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-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits' -> 'wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.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-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
WCS-calibrated image found: wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
Checking if the catalog wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
WCS catalog name: wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=477, bad_region=0, passed=8960
Got 8960 stars (including 8469 good ones) from the SExtractor catalog wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat
util/solve_plate_with_UCAC5 got 8960 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 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 4870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 8960 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 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 8960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 8960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4870 stars left (next iteration limit 5357)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits N_match=4870 sigma_overall_arcsec=0.399 sigma_q1_arcsec=0.324 sigma_q2_arcsec=0.453 sigma_q3_arcsec=0.398 sigma_q4_arcsec=0.405 n_q1=1235 n_q2=1146 n_q3=1371 n_q4=1118 worst_quadrant_to_overall_ratio=1.134
WCS_HEADER_DIAG: file=Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits selection=current_pairs N_selected=4870 N_valid=4870 bias_ra_arcsec=0.026 bias_dec_arcsec=0.005 median_sep_arcsec=0.295 p95_sep_arcsec=1.347 n_q1=1235 n_q2=1146 n_q3=1371 n_q4=1118 occupied_cells_4x4=16/16
The image catalog is written to wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits -region wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.6uvZF306XE (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_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.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_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
Checking if the catalog wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
WCS catalog name: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=358, bad_region=1, passed=5437
Got 5437 stars (including 5070 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat
util/solve_plate_with_UCAC5 got 5437 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 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 491 to 549 (Dec 8.4 to 19.4)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 4860 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 5437 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
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 491 to 549 (Dec 8.4 to 19.4)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 5437 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 5437 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4860 stars left (next iteration limit 5346)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4860 robust_rms=13.834 arcsec worst_region_rms=27.618 arcsec outer_annulus_rms=27.618 arcsec
SIP_REFIT: SIP order 3 trial: matched=4860 robust_rms=0.427 arcsec worst_region_rms=0.854 arcsec outer_annulus_rms=0.854 arcsec
SIP_REFIT: SIP order 5 trial: matched=4860 robust_rms=0.252 arcsec worst_region_rms=0.289 arcsec outer_annulus_rms=0.289 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4860 robust_rms_before=0.893 arcsec robust_rms_before_corrected=0.272 arcsec robust_rms_after=0.252 arcsec worst_region_rms_before=0.340 worst_region_rms_after=0.289 outer_annulus_rms_before=0.916 outer_annulus_rms_after=0.289
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.sip_refit.XvwA7T/candidate.fits
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.sip_refit.XvwA7T/candidate.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:07:03.619 +13:59:16.41 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5437 stars ###
'wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.sip_refit.XvwA7T/candidate.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction_1653214.cat.log'
'wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.sip_refit.XvwA7T/candidate.wcscat.xy2sky.BmdwVj' -> 'vast_debug_catalog_after_xy2sky_correction_1653214.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.893 -> 0.252 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (cycle 1, search radius 3.0 arcsec, 4860 pairs from the previous matching)
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 491 to 549 (Dec 8.4 to 19.4)
Done reading UCAC5 zone files...
Matched 4705 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4705 pairs (4860 from the previous matching)
SIP_REFIT: SIP order 2 trial: matched=4705 robust_rms=13.822 arcsec worst_region_rms=27.550 arcsec outer_annulus_rms=27.550 arcsec
SIP_REFIT: SIP order 3 trial: matched=4705 robust_rms=0.427 arcsec worst_region_rms=0.838 arcsec outer_annulus_rms=0.838 arcsec
SIP_REFIT: SIP order 5 trial: matched=4705 robust_rms=0.251 arcsec worst_region_rms=0.288 arcsec outer_annulus_rms=0.288 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4705 robust_rms_before=0.252 arcsec robust_rms_before_corrected=0.252 arcsec robust_rms_after=0.251 arcsec worst_region_rms_before=0.288 worst_region_rms_after=0.288 outer_annulus_rms_before=0.288 outer_annulus_rms_after=0.288
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-region 0.288 vs 0.288 arcsec) - keeping the current solution
SIP_REFIT: the refit on the re-matched pairs was not applied - keeping the current solution
Accuracy estimation diagnostic: 4705 matched stars entering correct_measured_positions(), 5437 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4705 matched stars entering correct_measured_positions(), 5437 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
WCS_QUALITY_DIAG: file=fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits N_match=4705 sigma_overall_arcsec=0.267 sigma_q1_arcsec=0.272 sigma_q2_arcsec=0.292 sigma_q3_arcsec=0.250 sigma_q4_arcsec=0.252 n_q1=1078 n_q2=1288 n_q3=1144 n_q4=1195 worst_quadrant_to_overall_ratio=1.094
WCS_HEADER_DIAG: file=fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits selection=current_pairs N_selected=4705 N_valid=4705 bias_ra_arcsec=-0.003 bias_dec_arcsec=0.005 median_sep_arcsec=0.212 p95_sep_arcsec=0.563 n_q1=1078 n_q2=1288 n_q3=1144 n_q4=1195 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits -region wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.TD2aUjvd7v (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_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.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_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
Checking if the catalog wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
WCS catalog name: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=360, bad_region=0, passed=5442
Got 5442 stars (including 5074 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat
util/solve_plate_with_UCAC5 got 5442 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 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 491 to 549 (Dec 8.4 to 19.4)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 4866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 5442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 491 to 549 (Dec 8.4 to 19.4)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 5442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 5442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4865 stars left (next iteration limit 5352)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4865 robust_rms=13.768 arcsec worst_region_rms=27.544 arcsec outer_annulus_rms=27.544 arcsec
SIP_REFIT: SIP order 3 trial: matched=4865 robust_rms=0.433 arcsec worst_region_rms=0.787 arcsec outer_annulus_rms=0.787 arcsec
SIP_REFIT: SIP order 5 trial: matched=4865 robust_rms=0.264 arcsec worst_region_rms=0.290 arcsec outer_annulus_rms=0.287 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4865 robust_rms_before=0.904 arcsec robust_rms_before_corrected=0.283 arcsec robust_rms_after=0.264 arcsec worst_region_rms_before=0.340 worst_region_rms_after=0.290 outer_annulus_rms_before=0.919 outer_annulus_rms_after=0.287
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.sip_refit.EnSuiY/candidate.fits
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.sip_refit.EnSuiY/candidate.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:07:01.328 +13:59:49.83 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5442 stars ###
'wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.sip_refit.EnSuiY/candidate.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction_1653210.cat.log'
'wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.sip_refit.EnSuiY/candidate.wcscat.xy2sky.EiJ7NJ' -> 'vast_debug_catalog_after_xy2sky_correction_1653210.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.904 -> 0.264 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (cycle 1, search radius 3.0 arcsec, 4865 pairs from the previous matching)
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 491 to 549 (Dec 8.4 to 19.4)
Done reading UCAC5 zone files...
Matched 4701 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4701 pairs (4865 from the previous matching)
SIP_REFIT: SIP order 2 trial: matched=4701 robust_rms=13.760 arcsec worst_region_rms=27.385 arcsec outer_annulus_rms=27.385 arcsec
SIP_REFIT: SIP order 3 trial: matched=4701 robust_rms=0.429 arcsec worst_region_rms=0.790 arcsec outer_annulus_rms=0.790 arcsec
SIP_REFIT: SIP order 5 trial: matched=4701 robust_rms=0.264 arcsec worst_region_rms=0.290 arcsec outer_annulus_rms=0.284 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4701 robust_rms_before=0.263 arcsec robust_rms_before_corrected=0.263 arcsec robust_rms_after=0.264 arcsec worst_region_rms_before=0.290 worst_region_rms_after=0.290 outer_annulus_rms_before=0.283 outer_annulus_rms_after=0.284
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.sip_refit.WAkBrU/candidate.fits
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.sip_refit.WAkBrU/candidate.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:07:01.328 +13:59:49.83 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5442 stars ###
'wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.sip_refit.WAkBrU/candidate.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction_1654000.cat.log'
'wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.sip_refit.WAkBrU/candidate.wcscat.xy2sky.0xXiyQ' -> 'vast_debug_catalog_after_xy2sky_correction_1654000.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.263 -> 0.264 arcsec)
Accuracy estimation diagnostic: 4701 matched stars entering correct_measured_positions(), 5442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4701 matched stars entering correct_measured_positions(), 5442 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
WCS_QUALITY_DIAG: file=fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits N_match=4701 sigma_overall_arcsec=0.277 sigma_q1_arcsec=0.281 sigma_q2_arcsec=0.305 sigma_q3_arcsec=0.266 sigma_q4_arcsec=0.262 n_q1=1059 n_q2=1304 n_q3=1144 n_q4=1194 worst_quadrant_to_overall_ratio=1.099
WCS_HEADER_DIAG: file=fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits selection=current_pairs N_selected=4701 N_valid=4701 bias_ra_arcsec=-0.004 bias_dec_arcsec=0.006 median_sep_arcsec=0.221 p95_sep_arcsec=0.581 n_q1=1059 n_q2=1304 n_q3=1144 n_q4=1194 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits -region wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits to local_wcs_cache/
'wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits' -> 'local_wcs_cache/wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits'
Saving the final (post-refit) wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits to local_wcs_cache/
'wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits' -> 'local_wcs_cache/wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits'
Saving the final (post-refit) wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits to local_wcs_cache/
'wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits' -> 'local_wcs_cache/wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits'
Saving the final (post-refit) wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits to local_wcs_cache/
'wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits' -> 'local_wcs_cache/wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits sigma_overall=0.391 worst_q_ratio=1.097
ref2=Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits sigma_overall=0.399 worst_q_ratio=1.134
new1=fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits sigma_overall=0.267 worst_q_ratio=1.094
new2=fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits sigma_overall=0.277 worst_q_ratio=1.099
reference average sigma_overall=0.395 worst_q_ratio=1.1155
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963_astrometric_residuals.png (4869 matched stars from wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432_astrometric_residuals.png (4870 matched stars from wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242_astrometric_residuals.png (4705 matched stars from wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.21 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243_astrometric_residuals.png (4701 matched stars from wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.22 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits'
Saving fully-calibrated image wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits'
Preparing the HTML report for the field Peg-10-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:37:36.14 +12:35:57.9: 10.07 +/- 0.00 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:37:36.14 +12:35:57.9: 10.07 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.07 +/- 0.00
Forced photometry filter REJECTED candidate at 23:37:36.14 +12:35:57.9: ref_mag=10.07 +/- 0.00 new_mean_mag=10.2755 delta=-0.20 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20348_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 20348_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20374_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 20374_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 23:36:10.23 +09:48:58.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08315_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 08315_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 22:44:53.30 +18:06:55.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05645_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 05645_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 23:04:11.49 +15:18:11.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Peg-10-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
SExtractor catalog cache: saved Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.cat to cache
SExtractor catalog cache: saved Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Creating symlink local_wcs_cache/wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
Checking 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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits exists and is non-empty
wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits exists and is non-empty
wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits exists and is non-empty
wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits (1st reference image)
verification OK: wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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: 23:06:39.243 +14:00:09.40 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-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits (1st new image)
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:07:03.619 +13:59:16.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:06:39.243 +14:00:09.40
Second-epoch image center 23:07:03.619 +13:59:16.41
Angular distance between the image centers 0.0996 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits (2nd new image)
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:07:01.328 +13:59:49.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:06:39.243 +14:00:09.40
Second-epoch image center 23:07:01.328 +13:59:49.83
Angular distance between the image centers 0.0895 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 23:07:03.619 +13:59:16.41
Second-epoch second image center 23:07:01.328 +13:59:49.83
Angular distance between the image centers 0.01311 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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits &> /tmp/tmp.YaiOnAuWAw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits &> /tmp/tmp.Y9TSUCEtvp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits &> /tmp/tmp.eD0QVIqgsb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits &> /tmp/tmp.uaV2iVxvEt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits and wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits and wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
Found non-empty wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits and wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
The reference image (wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits) and catalog (wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat) found
'wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat' -> 'wcsmag.cat'
Read 52987 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.3668 to 354.8803 deg, Dec +8.6362 to +19.2696 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 338.3668 to 354.8803 deg, Dec 8.6362 to 19.2696 deg
Loaded 5972 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): 4571 out of 5107 total matches.
Matched with Tycho-2 5107 out of 52987 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.: -6.92
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.65
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.65
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 52987 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.3668 to 354.8803 deg, Dec +8.6362 to +19.2696 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 338.3668 to 354.8803 deg, Dec 8.6362 to 19.2696 deg
Loaded 5972 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): 4571 out of 5107 total matches.
Matched with Tycho-2 5107 out of 52987 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Forced-photometry filter: calibrated wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits -> calib.txt_param_ref_wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits (aperture=4.9)
Read 51434 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.3689 to 354.8805 deg, Dec +8.6361 to +19.2674 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 338.3689 to 354.8805 deg, Dec 8.6361 to 19.2674 deg
Loaded 5969 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): 4607 out of 5108 total matches.
Matched with Tycho-2 5108 out of 51434 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
Forced-photometry filter: calibrated wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits -> calib.txt_param_ref_wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits (aperture=4.9)
____ 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:
2.1 pix Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
2.1 pix Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
2.1 pix fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
2.1 pix fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
Limiting magnitude estimates:
15.7 mag. Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
15.6 mag. Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
15.0 mag. fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
15.0 mag. fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.YaiOnAuWAw (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits' -> 'wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
WCS-calibrated image found: wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
Checking if the catalog wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits
WCS catalog name: wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=24, blended=2646, bad_region=0, passed=52963
Got 52963 stars (including 50236 good ones) from the SExtractor catalog wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat
util/solve_plate_with_UCAC5 got 52963 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 4880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 4870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 52963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4880 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 52963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 52963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4868 stars left (next iteration limit 5357)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.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-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits N_match=4868 sigma_overall_arcsec=0.383 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.423 sigma_q3_arcsec=0.401 sigma_q4_arcsec=0.387 n_q1=1235 n_q2=1157 n_q3=1328 n_q4=1148 worst_quadrant_to_overall_ratio=1.104
WCS_HEADER_DIAG: file=Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits selection=current_pairs N_selected=4868 N_valid=4868 bias_ra_arcsec=0.012 bias_dec_arcsec=-0.008 median_sep_arcsec=0.292 p95_sep_arcsec=1.258 n_q1=1235 n_q2=1157 n_q3=1328 n_q4=1148 occupied_cells_4x4=16/16
The image catalog is written to wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits -region wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Y9TSUCEtvp (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.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-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits' -> 'wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.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-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
WCS-calibrated image found: wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
Checking if the catalog wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat corresponding to the image wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits
WCS catalog name: wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=17, blended=2452, bad_region=0, passed=51417
Got 51417 stars (including 48885 good ones) from the SExtractor catalog wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat
util/solve_plate_with_UCAC5 got 51417 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 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 4868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 51417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 51417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 51417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4868 stars left (next iteration limit 5354)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.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-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits N_match=4868 sigma_overall_arcsec=0.389 sigma_q1_arcsec=0.318 sigma_q2_arcsec=0.442 sigma_q3_arcsec=0.385 sigma_q4_arcsec=0.400 n_q1=1243 n_q2=1141 n_q3=1346 n_q4=1138 worst_quadrant_to_overall_ratio=1.137
WCS_HEADER_DIAG: file=Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits selection=current_pairs N_selected=4868 N_valid=4868 bias_ra_arcsec=0.031 bias_dec_arcsec=-0.005 median_sep_arcsec=0.291 p95_sep_arcsec=1.337 n_q1=1243 n_q2=1141 n_q3=1346 n_q4=1138 occupied_cells_4x4=16/16
The image catalog is written to wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits -region wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.eD0QVIqgsb (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_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.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_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
Checking if the catalog wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
WCS catalog name: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=5, blended=1187, bad_region=29, passed=35647
Got 35647 stars (including 34366 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat
util/solve_plate_with_UCAC5 got 35647 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 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 491 to 549 (Dec 8.3 to 19.4)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 35647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
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 491 to 549 (Dec 8.3 to 19.4)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 35647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 35647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4864 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.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=4864 robust_rms=13.659 arcsec worst_region_rms=28.653 arcsec outer_annulus_rms=28.653 arcsec
SIP_REFIT: SIP order 3 trial: matched=4864 robust_rms=0.424 arcsec worst_region_rms=0.894 arcsec outer_annulus_rms=0.894 arcsec
SIP_REFIT: SIP order 5 trial: matched=4864 robust_rms=0.248 arcsec worst_region_rms=0.291 arcsec outer_annulus_rms=0.291 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4864 robust_rms_before=0.249 arcsec robust_rms_before_corrected=0.261 arcsec robust_rms_after=0.248 arcsec worst_region_rms_before=0.291 worst_region_rms_after=0.291 outer_annulus_rms_before=0.291 outer_annulus_rms_after=0.291
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.291 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits worst_region_rms_kept=0.291 arcsec robust_rms_kept=0.249 arcsec matched=4864
WCS_QUALITY_DIAG: file=fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits N_match=4864 sigma_overall_arcsec=0.262 sigma_q1_arcsec=0.277 sigma_q2_arcsec=0.294 sigma_q3_arcsec=0.235 sigma_q4_arcsec=0.250 n_q1=1156 n_q2=1358 n_q3=1171 n_q4=1179 worst_quadrant_to_overall_ratio=1.123
WCS_HEADER_DIAG: file=fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits selection=current_pairs N_selected=4864 N_valid=4864 bias_ra_arcsec=-0.003 bias_dec_arcsec=0.011 median_sep_arcsec=0.212 p95_sep_arcsec=0.629 n_q1=1156 n_q2=1358 n_q3=1171 n_q4=1179 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits -region wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.uaV2iVxvEt (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_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.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_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
Checking if the catalog wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
WCS catalog name: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=9, blended=1220, bad_region=27, passed=35923
Got 35923 stars (including 34615 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat
util/solve_plate_with_UCAC5 got 35923 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 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 491 to 549 (Dec 8.3 to 19.4)
Done reading UCAC5 zone files...
Matched 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 35923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
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 491 to 549 (Dec 8.3 to 19.4)
Done reading UCAC5 zone files...
Matched 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 35923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 35923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4864 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.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=4864 robust_rms=13.563 arcsec worst_region_rms=28.392 arcsec outer_annulus_rms=28.392 arcsec
SIP_REFIT: SIP order 3 trial: matched=4864 robust_rms=0.430 arcsec worst_region_rms=0.863 arcsec outer_annulus_rms=0.863 arcsec
SIP_REFIT: SIP order 5 trial: matched=4864 robust_rms=0.260 arcsec worst_region_rms=0.285 arcsec outer_annulus_rms=0.285 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4864 robust_rms_before=0.261 arcsec robust_rms_before_corrected=0.267 arcsec robust_rms_after=0.260 arcsec worst_region_rms_before=0.284 worst_region_rms_after=0.285 outer_annulus_rms_before=0.283 outer_annulus_rms_after=0.285
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.284 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits worst_region_rms_kept=0.284 arcsec robust_rms_kept=0.261 arcsec matched=4864
WCS_QUALITY_DIAG: file=fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits N_match=4864 sigma_overall_arcsec=0.271 sigma_q1_arcsec=0.274 sigma_q2_arcsec=0.294 sigma_q3_arcsec=0.254 sigma_q4_arcsec=0.263 n_q1=1146 n_q2=1364 n_q3=1163 n_q4=1191 worst_quadrant_to_overall_ratio=1.086
WCS_HEADER_DIAG: file=fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits selection=current_pairs N_selected=4864 N_valid=4864 bias_ra_arcsec=-0.002 bias_dec_arcsec=0.010 median_sep_arcsec=0.220 p95_sep_arcsec=0.642 n_q1=1146 n_q2=1364 n_q3=1163 n_q4=1191 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits -region wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.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_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-51-55_20.00sec_-0.00C_LIGHTs_0242.fits
Saving fully-calibrated image wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.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_2026-10-27_CI_Peg-10-Q1b1x1_235334_TTUQ1b1x1_1575959_3Hj3smed/wcs_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243.fits
Preparing the HTML report for the field Peg-10-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:36:18.40 +12:10:30.8: 12.80 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:48:40.07 +17:53:57.9: 13.94 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:39:13.90 +17:58:46.3: 12.98 +/- 0.03 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:12:07.43 +14:25:38.5: 14.10 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:28:04.68 +10:05:18.4: 13.51 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:53:34.58 +18:39:53.7: 12.90 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:00:24.26 +16:44:31.8: 12.70 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:47:58.54 +18:33:50.8: 13.36 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:37:36.13 +12:35:57.9: 10.22 +/- 0.00 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:33:36.44 +10:30:00.3: 12.84 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:48:40.07 +17:53:57.9: 13.89 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:36:18.40 +12:10:30.8: 12.87 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:33:36.44 +10:30:00.3: 12.92 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:00:24.26 +16:44:31.8: 12.79 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:37:36.13 +12:35:57.9: 10.22 +/- 0.00 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:28:04.68 +10:05:18.4: 13.44 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:12:07.43 +14:25:38.5: 14.07 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:39:13.90 +17:58:46.3: 12.96 +/- 0.03 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:53:34.58 +18:39:53.7: 12.82 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:47:58.54 +18:33:50.8: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.04
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry filter REJECTED candidate at 22:48:40.07 +17:53:57.9: ref_mag=13.92 +/- 0.04 new_mean_mag=14.2132 delta=-0.30 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:33:36.44 +10:30:00.3: ref_mag=12.88 +/- 0.02 new_mean_mag=12.8315 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 10.22 +/- 0.00
Forced photometry filter REJECTED candidate at 23:36:18.40 +12:10:30.8: ref_mag=12.83 +/- 0.02 new_mean_mag=12.8791 delta=-0.05 (need > 0.90)
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Forced photometry filter REJECTED candidate at 23:00:24.26 +16:44:31.8: ref_mag=12.74 +/- 0.01 new_mean_mag=12.9804 delta=-0.24 (need > 0.90)
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter REJECTED candidate at 23:37:36.13 +12:35:57.9: ref_mag=10.22 +/- 0.00 new_mean_mag=10.3279 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 14.08 +/- 0.04
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Forced photometry filter REJECTED candidate at 23:28:04.68 +10:05:18.4: ref_mag=13.47 +/- 0.03 new_mean_mag=13.6302 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:47:58.54 +18:33:50.8: ref_mag=13.35 +/- 0.03 new_mean_mag=13.6603 delta=-0.31 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:12:07.43 +14:25:38.5: ref_mag=14.08 +/- 0.04 new_mean_mag=14.1696 delta=-0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:39:13.90 +17:58:46.3: ref_mag=12.97 +/- 0.02 new_mean_mag=13.2124 delta=-0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:53:34.58 +18:39:53.7: ref_mag=12.86 +/- 0.02 new_mean_mag=13.3255 delta=-0.47 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:31:44.57 +09:19:43.5: 13.57 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:41:11.46 +15:29:42.9: 12.63 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:32:59.65 +08:47:06.6: 13.30 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:35:09.48 +09:49:47.5: 13.30 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:44:24.75 +14:16:52.6: 12.63 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:32:45.93 +14:19:33.0: 13.42 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:37:34.52 +15:28:35.8: 13.17 +/- 0.03 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:54:55.87 +15:21:55.6: 13.48 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:31:44.57 +09:19:43.5: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Forced photometry filter REJECTED candidate at 23:31:44.57 +09:19:43.5: ref_mag=13.59 +/- 0.03 new_mean_mag=13.3158 delta=0.28 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:44:24.75 +14:16:52.6: 12.67 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:32:59.65 +08:47:06.6: 13.25 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:41:11.46 +15:29:42.9: 12.64 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:35:09.48 +09:49:47.5: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Forced photometry filter REJECTED candidate at 22:44:24.75 +14:16:52.6: ref_mag=12.65 +/- 0.02 new_mean_mag=12.5933 delta=0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:32:59.65 +08:47:06.6: ref_mag=13.28 +/- 0.03 new_mean_mag=13.3021 delta=-0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:41:11.46 +15:29:42.9: ref_mag=12.63 +/- 0.02 new_mean_mag=12.6592 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Forced photometry filter REJECTED candidate at 23:35:09.48 +09:49:47.5: ref_mag=13.31 +/- 0.03 new_mean_mag=13.1269 delta=0.18 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:44:17.41 +11:56:13.8: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:37:34.52 +15:28:35.8: 13.15 +/- 0.03 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:32:45.93 +14:19:33.0: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter REJECTED candidate at 22:37:34.52 +15:28:35.8: ref_mag=13.16 +/- 0.02 new_mean_mag=13.3991 delta=-0.24 (need > 0.90)
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Forced photometry filter REJECTED candidate at 23:32:45.93 +14:19:33.0: ref_mag=13.41 +/- 0.03 new_mean_mag=13.4003 delta=0.01 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:54:55.87 +15:21:55.6: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Forced photometry filter REJECTED candidate at 22:54:55.87 +15:21:55.6: ref_mag=13.50 +/- 0.03 new_mean_mag=13.5953 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:47:07.56 +10:48:04.7: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:44:17.41 +11:56:13.8: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:47:27.69 +14:07:50.9: 13.57 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:44:33.97 +14:16:41.5: 13.48 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:16:51.23 +15:34:03.3: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:12:25.31 +18:20:34.1: 13.60 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:47:07.56 +10:48:04.7: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:14:12.70 +16:32:36.2: 14.05 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:37:32.49 +09:54:15.9: 14.60 +/- 0.12 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:10:54.37 +16:47:17.5: 14.05 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:47:27.69 +14:07:50.9: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Forced photometry filter REJECTED candidate at 22:47:27.69 +14:07:50.9: ref_mag=13.55 +/- 0.03 new_mean_mag=13.7241 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:16:51.23 +15:34:03.3: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:44:33.97 +14:16:41.5: 13.49 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:12:25.31 +18:20:34.1: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.04
Forced photometry filter REJECTED candidate at 22:44:33.97 +14:16:41.5: ref_mag=13.49 +/- 0.04 new_mean_mag=13.6811 delta=-0.19 (need > 0.90)
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter REJECTED candidate at 23:12:25.31 +18:20:34.1: ref_mag=13.62 +/- 0.03 new_mean_mag=13.8920 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:27:42.71 +18:05:13.3: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:14:12.70 +16:32:36.2: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.05
Forced photometry filter REJECTED candidate at 23:14:12.70 +16:32:36.2: ref_mag=14.03 +/- 0.05 new_mean_mag=14.1224 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:10:54.37 +16:47:17.5: 14.12 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:37:32.49 +09:54:15.9: 14.51 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.04
Forced photometry filter REJECTED candidate at 23:10:54.37 +16:47:17.5: ref_mag=14.08 +/- 0.04 new_mean_mag=14.1878 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 14.56 +/- 0.08
Forced photometry filter REJECTED candidate at 23:37:32.49 +09:54:15.9: ref_mag=14.56 +/- 0.08 new_mean_mag=14.2681 delta=0.29 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:27:42.71 +18:05:13.3: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:08:59.24 +18:20:23.3: 13.91 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:55:06.64 +16:53:29.2: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:08:59.24 +18:20:23.3: 13.84 +/- 0.05 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:55:06.64 +16:53:29.2: 15.93 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.88 +/- 0.04
Forced photometry filter REJECTED candidate at 23:08:59.24 +18:20:23.3: ref_mag=13.88 +/- 0.04 new_mean_mag=14.2339 delta=-0.36 (need > 0.90)
Adding exclusion_list_local.txt__out66867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67315.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 34s
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: 3s
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Considering the candidate 66186_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66186_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66193_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66193_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66198_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66198_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66201_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66201_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66202_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66202_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66206_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66206_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66207_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66207_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66208_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66208_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66209_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66209_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66210_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66210_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66405_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66405_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 22:54:43.01 +16:58:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66418_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66418_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 22:41:30.41 +10:47:29.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 66477_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66477_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 22:40:47.52 +14:32:03.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 66510_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66510_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66526_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66526_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66570_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66570_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 23:04:53.54 +15:14:32.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 66622_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66622_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66663_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66663_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 23:28:14.05 +18:19:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66691_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66691_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66705_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66705_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66706_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66706_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66768_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66768_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 23:06:15.71 +18:29:39.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 66782_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66782_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 22:44:35.49 +14:17:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66788_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66788_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66843_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66843_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66851_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66851_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 23:22:38.16 +11:11:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66867_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
Preparing report for the candidate 66867_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
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Considering the candidate 66913_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
Preparing report for the candidate 66913_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
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Considering the candidate 66929_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66929_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66943_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66943_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 66988_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 66988_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 22:41:51.88 +10:31:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66999_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
Preparing report for the candidate 66999_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
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Considering the candidate 67027_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 67027_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 67103_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 67103_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 67133_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 67133_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 23:05:18.76 +10:53:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67153_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 67153_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 67185_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 67185_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 67194_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
Preparing report for the candidate 67194_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
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Considering the candidate 67199_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 67199_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
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Considering the candidate 67315_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
Preparing report for the candidate 67315_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
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Considering the candidate 04390_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 04390_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 23:36:10.23 +09:48:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50100_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 50100_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
Rejecting candidate due to large distance (47.5") between the two second-epoch detections
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Considering the candidate 35336_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 35336_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
**** FOUND 23:04:11.49 +15:18:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40985_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243
The candidate 40985_fd_Peg-10-Q1b1x1_2026-10-27_23-52-50_20.00sec_-0.00C_LIGHTs_0243 did not pass the final checks
