This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz
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 11.3615 2461324.8615 10.70 23:01:46.75 +13:05:14.1
85.96190 -41.77978 galactic Peg Second-epoch detections are separated by 0.5" and 10.2 pix
The object was found in VSX 0" V0561 Peg
Type: M
# Max. Min./Amp. JD0 Period
10.600 V 13.500 V 2453635.00000 300.000000000000 Np
The object was not found in astcheck.
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:01:46.75 +13:05:14.1: 11.64 +/- 0.01 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:01:46.75 +13:05:14.1: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0561 Peg,2461324.8615,10.70,0.05,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
V0561 Peg 20261011.3615 10.70CV 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 11.3615 2461324.8615 11.76 22:37:21.10 +10:32:55.3
77.59930 -40.23669 galactic Peg Second-epoch detections are separated by 0.4" and 10.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.198 Ampella -0 -0 1 10.9 0 0
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:37:21.10 +10:32:55.3: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:37:21.10 +10:32:55.3: 15.65 +/- 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,2461324.8615,11.76,0.05,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 20261011.3615 11.76CV 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 11.3615 2461324.8615 13.24 22:50:04.20 +13:20:15.6
83.04886 -39.95417 galactic Peg Second-epoch detections are separated by 0.6" and 10.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.170 Maria 0 0 0 13.2 -0 -0
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:50:04.20 +13:20:15.6: 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 22:50:04.20 +13:20:15.6: 15.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461324.8615,13.24,0.05,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 20261011.3615 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3615 2461324.8615 13.34 22:45:22.17 +14:36:42.9
82.82973 -38.25267 galactic Peg Second-epoch detections are separated by 1.8" and 10.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.978 Aidamina 0 -0 0 13.4 -0 0
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:45:22.17 +14:36:42.9: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:45:22.17 +14:36:42.9: 15.83 +/- 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,2461324.8615,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261011.3615 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.3615 2461324.8615 13.62 23:24:33.19 +17:05:26.1
94.97296 -41.01670 galactic Peg Second-epoch detections are separated by 1.7" and 10.1 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 13.6 -0 0
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:24:33.19 +17:05:26.1: 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 23:24:33.19 +17:05:26.1: 15.99 +/- 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,2461324.8615,13.62,0.05,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 20261011.3615 13.62CV 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 11.3615 2461324.8615 14.13 23:20:55.64 +10:22:10.9
89.54325 -46.55102 galactic Peg Second-epoch detections are separated by 1.0" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1001 Gaussia -0 -0 0 14.2 -0 0
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:20:55.64 +10:22:10.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:20:55.64 +10:22:10.9: 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,2461324.8615,14.13,0.05,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 20261011.3615 14.13CV 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: 2461324.86179903 11.10.2026 08:40:49.436 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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): 8758
Objects passed selection criteria: 8736
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 7133.75
Average stars matched: 6989.25 (97.9744 %)
Memory usage VmPeak: 234916 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Oct 11 03:48:15 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: 2461324.86179903 11.10.2026 08:40:49.436 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 41
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: 12 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): 49621
Objects passed selection criteria: 49504
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: 43719.8
Average stars matched: 42378.5 (96.9322 %)
Memory usage VmPeak: 270520 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Oct 11 03:49:08 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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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: 2461324.86120781
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_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits exists and is non-empty
wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits (1st new image)
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
Image size: 941.5'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:06:44.541 +13:58:44.19 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 23:06:44.541 +13:58:44.19
Angular distance between the image centers 0.0319 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits (2nd new image)
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
Image size: 941.6'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:06:47.637 +13:58:03.39 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 23:06:47.637 +13:58:03.39
Angular distance between the image centers 0.0488 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 23:06:44.541 +13:58:44.19
Second-epoch second image center 23:06:47.637 +13:58:03.39
Angular distance between the image centers 0.01689 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.TK87MGmsWN
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.SLq4VtKkEo
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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits &> /tmp/tmp.vWzLqfBkVg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits &> /tmp/tmp.LNzjjuvs26
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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 3 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_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
2.2 pix fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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
14.8 mag. fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
14.8 mag. fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.6 (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.TK87MGmsWN (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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/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
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.SLq4VtKkEo (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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/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
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.vWzLqfBkVg (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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
Checking if the catalog wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.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_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
WCS catalog name: wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.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=256, bad_region=0, passed=5354
Got 5354 stars (including 5092 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat
util/solve_plate_with_UCAC5 got 5354 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 19.5)
Done reading UCAC5 zone files...
Matched 4894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 4886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 5354 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 8.3 to 19.5)
Done reading UCAC5 zone files...
Matched 4894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 5354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 5354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4885 stars left (next iteration limit 5373)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4885 robust_rms=12.972 arcsec worst_region_rms=27.436 arcsec outer_annulus_rms=27.436 arcsec
SIP_REFIT: SIP order 3 trial: matched=4885 robust_rms=0.445 arcsec worst_region_rms=0.995 arcsec outer_annulus_rms=0.995 arcsec
SIP_REFIT: SIP order 5 trial: matched=4885 robust_rms=0.264 arcsec worst_region_rms=0.324 arcsec outer_annulus_rms=0.324 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4885 robust_rms_before=0.901 arcsec robust_rms_before_corrected=0.277 arcsec robust_rms_after=0.264 arcsec worst_region_rms_before=0.360 worst_region_rms_after=0.324 outer_annulus_rms_before=0.924 outer_annulus_rms_after=0.324
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.360 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits worst_region_rms_kept=0.360 arcsec robust_rms_kept=0.277 arcsec matched=4885
WCS_QUALITY_DIAG: file=fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits N_match=4885 sigma_overall_arcsec=0.289 sigma_q1_arcsec=0.293 sigma_q2_arcsec=0.309 sigma_q3_arcsec=0.262 sigma_q4_arcsec=0.264 n_q1=1193 n_q2=1442 n_q3=1221 n_q4=1029 worst_quadrant_to_overall_ratio=1.069
The image catalog is written to wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits -region wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.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.LNzjjuvs26 (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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
Checking if the catalog wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
WCS catalog name: wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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=257, bad_region=0, passed=5050
Got 5050 stars (including 4791 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits.wcscat
util/solve_plate_with_UCAC5 got 5050 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4689 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4676 matched stars entering correct_measured_positions(), 4676 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4675 matched stars entering correct_measured_positions(), 5047 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 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4689 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4677 matched stars entering correct_measured_positions(), 5047 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4676 matched stars entering correct_measured_positions(), 5047 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4676 stars left (next iteration limit 5142)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4676 robust_rms=13.130 arcsec worst_region_rms=27.213 arcsec outer_annulus_rms=27.213 arcsec
SIP_REFIT: SIP order 3 trial: matched=4676 robust_rms=0.474 arcsec worst_region_rms=0.881 arcsec outer_annulus_rms=0.881 arcsec
SIP_REFIT: SIP order 5 trial: matched=4676 robust_rms=0.281 arcsec worst_region_rms=0.330 arcsec outer_annulus_rms=0.330 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4676 robust_rms_before=0.895 arcsec robust_rms_before_corrected=0.290 arcsec robust_rms_after=0.281 arcsec worst_region_rms_before=0.363 worst_region_rms_after=0.330 outer_annulus_rms_before=0.926 outer_annulus_rms_after=0.330
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.363 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits worst_region_rms_kept=0.363 arcsec robust_rms_kept=0.290 arcsec matched=4676
WCS_QUALITY_DIAG: file=fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits N_match=4676 sigma_overall_arcsec=0.299 sigma_q1_arcsec=0.302 sigma_q2_arcsec=0.309 sigma_q3_arcsec=0.274 sigma_q4_arcsec=0.276 n_q1=1171 n_q2=1406 n_q3=1237 n_q4=862 worst_quadrant_to_overall_ratio=1.034
The image catalog is written to wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits -region wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits to local_wcs_cache/
'wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits' -> 'local_wcs_cache/wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits'
Saving the final (post-refit) wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits to local_wcs_cache/
'wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits' -> 'local_wcs_cache/wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits sigma_overall=0.289 worst_q_ratio=1.069
new2=fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits sigma_overall=0.299 worst_q_ratio=1.034
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_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261_astrometric_residuals.png (4885 matched stars from wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262_astrometric_residuals.png (4676 matched stars from wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits'
Saving fully-calibrated image wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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 23:37:34.85 +12:35:49.9: 10.09 +/- 0.00 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:01:46.75 +13:05:14.1: 11.64 +/- 0.01 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:37:34.85 +12:35:49.9: 10.09 +/- 0.00 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:01:46.75 +13:05:14.1: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.09 +/- 0.00
Forced photometry reference-image weighted average: 11.63 +/- 0.01
Forced photometry filter REJECTED candidate at 23:37:34.85 +12:35:49.9: ref_mag=10.09 +/- 0.00 new_mean_mag=10.4954 delta=-0.41 (need > 0.90)
Forced photometry filter KEPT candidate at 23:01:46.75 +13:05:14.1: ref_mag=11.63 +/- 0.01 new_mean_mag=10.6865 delta=0.94 (need > 0.90)
Adding exclusion_list_local.txt__out03748.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20348_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 20348_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 08315_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 08315_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 22:44:53.31 +18:06:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03748_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
Preparing report for the candidate 03748_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
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 ####
23:01:46.75 +13:05:14.1
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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits exists and is non-empty
wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits (1st new image)
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
Image size: 941.5'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:06:44.541 +13:58:44.19 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 23:06:44.541 +13:58:44.19
Angular distance between the image centers 0.0319 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits (2nd new image)
verification OK: wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
Image size: 941.6'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:06:47.637 +13:58:03.39 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 23:06:47.637 +13:58:03.39
Angular distance between the image centers 0.0488 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 23:06:44.541 +13:58:44.19
Second-epoch second image center 23:06:47.637 +13:58:03.39
Angular distance between the image centers 0.01689 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.mqlpS8UoJK
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.S3FvmqSpfL
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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits &> /tmp/tmp.9yHvEtYRzg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits &> /tmp/tmp.wlGQk5YDC0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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 38 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
2.0 pix fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
2.0 pix fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
15.1 mag. fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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.mqlpS8UoJK (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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/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
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.S3FvmqSpfL (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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/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
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.9yHvEtYRzg (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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
Checking if the catalog wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.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_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
WCS catalog name: wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.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=13, blended=1210, bad_region=42, passed=36299
Got 36299 stars (including 34991 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat
util/solve_plate_with_UCAC5 got 36299 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 4863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 36299 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 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 36299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 36299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4863 stars left (next iteration limit 5349)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.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=4863 robust_rms=12.805 arcsec worst_region_rms=27.890 arcsec outer_annulus_rms=27.890 arcsec
SIP_REFIT: SIP order 3 trial: matched=4863 robust_rms=0.438 arcsec worst_region_rms=1.114 arcsec outer_annulus_rms=1.114 arcsec
SIP_REFIT: SIP order 5 trial: matched=4863 robust_rms=0.261 arcsec worst_region_rms=0.322 arcsec outer_annulus_rms=0.322 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4863 robust_rms_before=0.901 arcsec robust_rms_before_corrected=0.266 arcsec robust_rms_after=0.261 arcsec worst_region_rms_before=0.347 worst_region_rms_after=0.322 outer_annulus_rms_before=0.914 outer_annulus_rms_after=0.322
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.347 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits worst_region_rms_kept=0.347 arcsec robust_rms_kept=0.266 arcsec matched=4863
WCS_QUALITY_DIAG: file=fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits N_match=4863 sigma_overall_arcsec=0.272 sigma_q1_arcsec=0.276 sigma_q2_arcsec=0.293 sigma_q3_arcsec=0.256 sigma_q4_arcsec=0.244 n_q1=1238 n_q2=1447 n_q3=1165 n_q4=1013 worst_quadrant_to_overall_ratio=1.077
The image catalog is written to wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits -region wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.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.wlGQk5YDC0 (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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
Checking if the catalog wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits
WCS catalog name: wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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=1127, bad_region=44, passed=35364
Got 35364 stars (including 34131 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits.wcscat
util/solve_plate_with_UCAC5 got 35364 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 8.2 to 19.5)
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(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 35356 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 8.2 to 19.5)
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(), 35356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 35356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4865 stars left (next iteration limit 5351)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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=4865 robust_rms=12.677 arcsec worst_region_rms=28.508 arcsec outer_annulus_rms=28.508 arcsec
SIP_REFIT: SIP order 3 trial: matched=4865 robust_rms=0.464 arcsec worst_region_rms=1.025 arcsec outer_annulus_rms=1.025 arcsec
SIP_REFIT: SIP order 5 trial: matched=4865 robust_rms=0.279 arcsec worst_region_rms=0.331 arcsec outer_annulus_rms=0.331 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4865 robust_rms_before=0.898 arcsec robust_rms_before_corrected=0.281 arcsec robust_rms_after=0.279 arcsec worst_region_rms_before=0.348 worst_region_rms_after=0.331 outer_annulus_rms_before=0.925 outer_annulus_rms_after=0.331
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.348 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits worst_region_rms_kept=0.348 arcsec robust_rms_kept=0.281 arcsec matched=4865
WCS_QUALITY_DIAG: file=fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits N_match=4865 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.295 sigma_q2_arcsec=0.301 sigma_q3_arcsec=0.270 sigma_q4_arcsec=0.267 n_q1=1284 n_q2=1476 n_q3=1246 n_q4=859 worst_quadrant_to_overall_ratio=1.052
The image catalog is written to wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits -region wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-39-58_20.00sec_-0.00C_LIGHTs_0261.fits
Saving fully-calibrated image wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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_2026-10-11_CI_Peg-10-Q1b1x1_034152_TTUQ1b1x1_2811828_YvJIR5tz/wcs_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262.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 23:33:36.42 +10:30:01.1: 12.85 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:55:54.74 +15:29:18.4: 14.19 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:00:24.29 +16:44:31.7: 12.67 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:36:18.46 +12:10:29.6: 12.76 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:37:36.10 +12:35:57.8: 10.20 +/- 0.00 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:55:44.11 +17:57:04.1: 12.78 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:36:48.99 +09:41:56.6: 12.20 +/- 0.01 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:00:15.12 +17:08:46.5: 14.22 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:24:48.07 +17:49:13.3: 14.22 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:01:01.97 +18:41:35.9: 13.43 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:00:24.29 +16:44:31.7: 12.77 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:55:44.11 +17:57:04.1: 12.77 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:37:36.10 +12:35:57.8: 10.20 +/- 0.00 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:55:54.74 +15:29:18.4: 14.16 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:24:48.07 +17:49:13.3: 14.31 +/- 0.08 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:33:36.42 +10:30:01.1: 12.93 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:36:48.99 +09:41:56.6: 12.26 +/- 0.01 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:01:01.97 +18:41:35.9: 13.52 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:36:18.46 +12:10:29.6: 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 23:00:15.12 +17:08:46.5: 14.25 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry reference-image weighted average: 14.26 +/- 0.05
Forced photometry filter REJECTED candidate at 23:00:24.29 +16:44:31.7: ref_mag=12.72 +/- 0.01 new_mean_mag=12.7937 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Forced photometry reference-image weighted average: 10.20 +/- 0.00
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Forced photometry filter REJECTED candidate at 23:24:48.07 +17:49:13.3: ref_mag=14.26 +/- 0.05 new_mean_mag=14.7239 delta=-0.47 (need > 0.90)
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Forced photometry reference-image weighted average: 14.23 +/- 0.05
Forced photometry reference-image weighted average: 14.18 +/- 0.05
Forced photometry filter REJECTED candidate at 22:55:44.11 +17:57:04.1: ref_mag=12.77 +/- 0.01 new_mean_mag=13.1199 delta=-0.35 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:37:36.10 +12:35:57.8: ref_mag=10.20 +/- 0.00 new_mean_mag=10.6049 delta=-0.40 (need > 0.90)
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter REJECTED candidate at 23:36:18.46 +12:10:29.6: ref_mag=12.79 +/- 0.01 new_mean_mag=13.0529 delta=-0.27 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:33:36.42 +10:30:01.1: ref_mag=12.89 +/- 0.02 new_mean_mag=12.8860 delta=0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:01:01.97 +18:41:35.9: ref_mag=13.48 +/- 0.03 new_mean_mag=13.8312 delta=-0.35 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:00:15.12 +17:08:46.5: ref_mag=14.23 +/- 0.05 new_mean_mag=14.4402 delta=-0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:55:54.74 +15:29:18.4: ref_mag=14.18 +/- 0.05 new_mean_mag=14.1817 delta=-0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:36:48.99 +09:41:56.6: ref_mag=12.23 +/- 0.01 new_mean_mag=12.3944 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:50:04.20 +13:20:15.6: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:45:22.17 +14:36:42.9: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:41:11.43 +15:29:42.7: 12.62 +/- 0.02 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:37:21.10 +10:32:55.3: 15.67 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:35:09.58 +09:49:46.9: 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 23:32:59.65 +08:47:04.9: 13.27 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:24:33.19 +17:05:26.1: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:37:34.45 +15:28:36.1: 13.21 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 22:54:55.87 +15:21:55.2: 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 22:37:21.10 +10:32:55.3: 15.65 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:45:22.17 +14:36:42.9: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:24:33.19 +17:05:26.1: 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 22:50:04.20 +13:20:15.6: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:37:34.45 +15:28:36.1: 13.19 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:32:59.65 +08:47:04.9: 13.24 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:54:55.87 +15:21:55.2: 13.51 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:35:09.58 +09:49:46.9: 13.31 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:41:11.43 +15:29:42.7: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Forced photometry filter REJECTED candidate at 22:54:55.87 +15:21:55.2: ref_mag=13.49 +/- 0.03 new_mean_mag=13.3456 delta=0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:35:09.58 +09:49:46.9: ref_mag=13.30 +/- 0.03 new_mean_mag=13.1006 delta=0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:37:34.45 +15:28:36.1: ref_mag=13.20 +/- 0.03 new_mean_mag=13.2703 delta=-0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:32:59.65 +08:47:04.9: ref_mag=13.26 +/- 0.03 new_mean_mag=13.1209 delta=0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:41:11.43 +15:29:42.7: ref_mag=12.63 +/- 0.02 new_mean_mag=12.6480 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:28:04.68 +10:05:18.6: 13.51 +/- 0.04 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:28:04.68 +10:05:18.6: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Forced photometry filter REJECTED candidate at 23:28:04.68 +10:05:18.6: ref_mag=13.47 +/- 0.03 new_mean_mag=13.3587 delta=0.11 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:10:54.42 +16:47:18.9: 14.02 +/- 0.06 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:31:44.61 +09:19:44.2: 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 22:50:57.81 +17:38:32.9: 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 23:20:55.64 +10:22:10.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:10:54.42 +16:47:18.9: 14.10 +/- 0.07 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:31:44.61 +09:19:44.2: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.04
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 22:50:57.81 +17:38:32.9: 14.01 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 23:10:54.42 +16:47:18.9: ref_mag=14.06 +/- 0.04 new_mean_mag=14.1605 delta=-0.10 (need > 0.90)
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter REJECTED candidate at 23:31:44.61 +09:19:44.2: ref_mag=13.60 +/- 0.03 new_mean_mag=13.3955 delta=0.20 (need > 0.90)
Forced photometry reference-image weighted average: 13.97 +/- 0.04
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:13:38.07 +14:11:11.1: 14.66 +/- 0.10 detection
Forced photometry filter REJECTED candidate at 22:50:57.81 +17:38:32.9: ref_mag=13.97 +/- 0.04 new_mean_mag=13.9168 delta=0.06 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:12:16.56 +14:14:24.1: 15.33 +/- 0.17 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:20:55.64 +10:22:10.9: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:13:38.07 +14:11:11.1: 14.56 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.07
Forced photometry filter REJECTED candidate at 23:13:38.07 +14:11:11.1: ref_mag=14.61 +/- 0.07 new_mean_mag=14.2163 delta=0.39 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:12:16.56 +14:14:24.1: 15.16 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.23 +/- 0.12
Forced photometry filter REJECTED candidate at 23:12:16.56 +14:14:24.1: ref_mag=15.23 +/- 0.12 new_mean_mag=14.6270 delta=0.61 (need > 0.90)
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:02:22.33 +14:40:10.6: 15.86 +/- 0.30 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:00:20.47 +18:27:12.2: 14.95 +/- 0.14 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-21_04-35-29_20.00sec_4.90C_LIGHT_0963.fits at 23:07:19.69 +16:34:44.8: 14.63 +/- 0.11 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:02:22.33 +14:40:10.6: 15.54 +/- 0.23 detection
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:00:20.47 +18:27:12.2: 14.93 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.66 +/- 0.18
Forced photometry filter KEPT candidate at 23:02:22.33 +14:40:10.6: ref_mag=15.66 +/- 0.18 new_mean_mag=14.6622 delta=1.00 (need > 0.90)
Forced photometry reference-image weighted average: 14.94 +/- 0.10
Forced photometry on wcs_Peg-10-Q1b1x1_2026-07-22_04-33-35_20.00sec_4.90C_LIGHT_0432.fits at 23:07:19.69 +16:34:44.8: 14.96 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 23:00:20.47 +18:27:12.2: ref_mag=14.94 +/- 0.10 new_mean_mag=14.6479 delta=0.29 (need > 0.90)
Forced photometry reference-image weighted average: 14.74 +/- 0.09
Forced photometry filter REJECTED candidate at 23:07:19.69 +16:34:44.8: ref_mag=14.74 +/- 0.09 new_mean_mag=14.6494 delta=0.09 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out67681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out66433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67548.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 66188_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66188_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66194_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66194_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66197_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66197_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66209_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66209_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66213_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66213_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66215_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66215_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66216_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66216_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66217_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66217_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66218_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66218_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66220_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66220_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66433_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
Preparing report for the candidate 66433_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
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Considering the candidate 66625_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66625_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66699_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66699_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 23:28:13.99 +18:19:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66793_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
Preparing report for the candidate 66793_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
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Considering the candidate 66843_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
Preparing report for the candidate 66843_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
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Considering the candidate 66856_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66856_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66883_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66883_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66904_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66904_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66924_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66924_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 66926_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
Preparing report for the candidate 66926_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
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Considering the candidate 66949_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 66949_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 22:44:35.47 +14:17:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67015_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 67015_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 67039_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 67039_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 67154_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 67154_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 23:22:38.15 +11:11:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67205_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 67205_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 67216_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 67216_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 23:05:18.75 +10:53:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67465_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 67465_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 67548_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
Preparing report for the candidate 67548_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
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Considering the candidate 67571_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 67571_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 23:05:07.19 +16:28:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67632_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 67632_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 67667_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 67667_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 67681_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 67681_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 23:02:22.33 +14:40:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 1.301 2816084784677043968 345.59278088995 +14.66986998193 15.1178 14.4605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67713_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 67713_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 67740_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 67740_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
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Considering the candidate 04390_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 04390_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 23:36:10.20 +09:48:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19883_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 19883_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 23:01:46.75 +13:05:14.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 40985_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 40985_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
**** FOUND 22:44:53.30 +18:06:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10407_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262
The candidate 10407_fd_Peg-10-Q1b1x1_2026-10-11_03-40-49_20.00sec_-0.00C_LIGHTs_0262 did not pass the final checks
