This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9467,14.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.4467 14.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9467,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.4467 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9467,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.4467 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3101438,2461149.9467,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3101438 20260419.4467 13.76CV 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
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
DocumentRef: VOTx3056389,2461149.9467,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3056389 20260419.4467 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3061337,2461149.9467,14.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3061337 20260419.4467 14.59CV 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 04 19.4467 2461149.9467 14.62 21:54:07.16 +33:47:18.2
85.76479 -15.99310 galactic Peg Second-epoch detections are separated by 3.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1948098763475099136 | 21:54:07.16 +33:47:18.2 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
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
Large-amplitude variable Gaia DR2 1948098763475099136,2461149.9467,14.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1948098763475099136 20260419.4467 14.62CV 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
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
DocumentRef: VOTx3066392,2461149.9467,14.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3066392 20260419.4467 14.66CV 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: 2461036.55507814 27.12.2025 01:19:08.751 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
First image: 2461036.55507814 27.12.2025 01:19:08.751 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
Last image: 2461149.94700348 19.04.2026 10:43:31.101 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 14
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.93
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: 8 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 17073
Objects passed selection criteria: 17004
Measurements per detected object (mean, median, min, max): 3.0 2.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 2.0 2 4
Average stars detected per image: 13076.2
Average stars matched: 11547.5 (88.309 %)
Memory usage VmPeak: 119820 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 05:46:47 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: 2461036.55507814 27.12.2025 01:19:08.751 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
First image: 2461036.55507814 27.12.2025 01:19:08.751 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
Last image: 2461149.94700348 19.04.2026 10:43:31.101 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 104
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
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: 58 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 109732
Objects passed selection criteria: 109431
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 84628.8
Average stars matched: 75468.2 (89.1757 %)
Memory usage VmPeak: 1954412 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 05:49:18 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
SExtractor catalog cache: saved Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat to cache
SExtractor catalog cache: saved Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.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-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461149.94640569
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits exists and is non-empty
Saving wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits to local_wcs_cache/
'wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits' -> 'local_wcs_cache/wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits'
wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits exists and is non-empty
Saving wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits to local_wcs_cache/
'wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits' -> 'local_wcs_cache/wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits'
wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits exists and is non-empty
Saving wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits to local_wcs_cache/
'wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits' -> 'local_wcs_cache/wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits'
wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits exists and is non-empty
Saving wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits to local_wcs_cache/
'wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits' -> 'local_wcs_cache/wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits (1st reference image)
verification OK: wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:00:00.402 +29:59:55.49 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits (1st new image)
verification OK: wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
Image size: 937.5'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:00:02.020 +30:00:24.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:00:00.402 +29:59:55.49
Second-epoch image center 22:00:02.020 +30:00:24.07
Angular distance between the image centers 0.0099 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits (2nd new image)
verification OK: wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
Image size: 937.5'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:00:01.095 +29:59:44.29 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:00:00.402 +29:59:55.49
Second-epoch image center 22:00:01.095 +29:59:44.29
Angular distance between the image centers 0.0040 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:00:02.020 +30:00:24.07
Second-epoch second image center 22:00:01.095 +29:59:44.29
Angular distance between the image centers 0.01154 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits &> /tmp/tmp.AEvUsAmg4M
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits &> /tmp/tmp.ZyNwo8rhpT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits &> /tmp/tmp.HMA21YlI5C
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits &> /tmp/tmp.SK9V3eJeJp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.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-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat
Found non-empty wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat
The reference image (wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits) and catalog (wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat) found
'wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat' -> 'wcsmag.cat'
Read 18030 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 320.5978 to 339.7068 deg, Dec +24.3174 to +35.3131 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 320.5978 to 339.7068 deg, Dec 24.3174 to 35.3131 deg
Loaded 15485 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): 10918 out of 11736 total matches.
Matched with Tycho-2 11736 out of 18030 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.949713
a=0.000000 b=1.000000 c=22.949713
From vast_summary.log: estimated ref. image limiting mag.: -7.93
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.02
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.02
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
2.4 pix Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
2.9 pix fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
2.9 pix fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
Limiting magnitude estimates:
15.0 mag. Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
15.0 mag. Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
14.7 mag. fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
14.7 mag. fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.AEvUsAmg4M (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-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.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-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.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-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits' -> 'wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
Checking if the catalog wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat corresponding to the image wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat corresponding to the image wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
WCS catalog name: wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1568, passed=18030
Got 18030 stars (including 16439 good ones) from the SExtractor catalog wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 18030 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 17529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 17527 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 17527 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits -region wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ZyNwo8rhpT (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-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.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-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.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-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits' -> 'wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
Checking if the catalog wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat corresponding to the image wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat corresponding to the image wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
WCS catalog name: wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1531, passed=18085
Got 18085 stars (including 16522 good ones) from the SExtractor catalog wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 18085 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 17575 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 17575 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 17575 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits -region wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.HMA21YlI5C (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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
WCS_IMAGE_NAME=wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
WCS-calibrated image found: wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
Checking if the catalog wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
WCS catalog name: wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1328, passed=15382
Got 15382 stars (including 14042 good ones) from the SExtractor catalog wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat
util/solve_plate_with_UCAC5 got 15382 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 15138 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 15137 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 15137 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits -region wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.SK9V3eJeJp (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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
WCS_IMAGE_NAME=wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
WCS-calibrated image found: wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
Checking if the catalog wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
WCS catalog name: wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1364, passed=15479
Got 15479 stars (including 14105 good ones) from the SExtractor catalog wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat
util/solve_plate_with_UCAC5 got 15479 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 15142 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 15144 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 15144 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits -region wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits'
Saving fully-calibrated image wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits'
Saving fully-calibrated image wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits'
Saving fully-calibrated image wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits'
Preparing the HTML report for the field Peg-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_apass.txt__out20826.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out24403.dat to exclusion_list_apass.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20826_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 20826_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:59:25.86 +28:20:36.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20828_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 20828_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:00:46.72 +33:17:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20829_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 20829_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:40:27.07 +33:18:30.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23667_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 23667_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:59:21.55 +34:09:55.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23738_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 23738_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:58:06.70 +27:23:56.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23984_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 23984_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:52:58.53 +33:48:28.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24403_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 24403_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:57:30.98 +27:13:30.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24439_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 24439_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:48:46.09 +27:23:39.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24574_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 24574_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:53:44.88 +32:02:13.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10579_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 10579_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:13:41.51 +29:22:51.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 12s
Prepared the HTML report for the field Peg-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
SExtractor catalog cache: saved Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat to cache
SExtractor catalog cache: saved Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.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-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
Creating symlink local_wcs_cache/wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits exists and is non-empty
wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits exists and is non-empty
wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits exists and is non-empty
wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits (1st reference image)
verification OK: wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 22:00:00.402 +29:59:55.49 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits (1st new image)
verification OK: wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
Image size: 937.5'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:00:02.020 +30:00:24.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:00:00.402 +29:59:55.49
Second-epoch image center 22:00:02.020 +30:00:24.07
Angular distance between the image centers 0.0099 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits (2nd new image)
verification OK: wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 937.5'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:00:01.095 +29:59:44.29 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:00:00.402 +29:59:55.49
Second-epoch image center 22:00:01.095 +29:59:44.29
Angular distance between the image centers 0.0040 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:00:02.020 +30:00:24.07
Second-epoch second image center 22:00:01.095 +29:59:44.29
Angular distance between the image centers 0.01154 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits &> /tmp/tmp.1liMt0y8NF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits &> /tmp/tmp.nnvzrGl4HF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits &> /tmp/tmp.YwOA5xdQf6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits &> /tmp/tmp.yta4TSR2KS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.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-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat
Found non-empty wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat
The reference image (wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits) and catalog (wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat) found
'wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat' -> 'wcsmag.cat'
Read 124319 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 320.5826 to 339.7068 deg, Dec +24.2972 to +35.3145 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 320.5826 to 339.7068 deg, Dec 24.2972 to 35.3145 deg
Loaded 15529 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): 9746 out of 12399 total matches.
Matched with Tycho-2 12399 out of 124319 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.773129
a=0.000000 b=1.000000 c=22.773129
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.21
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.21
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 83 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
2.2 pix Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
2.8 pix fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
2.8 pix fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
Limiting magnitude estimates:
15.2 mag. Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
15.2 mag. Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
14.7 mag. fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
14.7 mag. fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.1liMt0y8NF (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-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.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-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.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-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits' -> 'wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
Checking if the catalog wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat corresponding to the image wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat corresponding to the image wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
WCS catalog name: wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=12699, passed=124274
Got 124274 stars (including 111350 good ones) from the SExtractor catalog wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 124274 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 122154 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 122155 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 122155 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits -region wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nnvzrGl4HF (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-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.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-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.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-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits' -> 'wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
Checking if the catalog wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat corresponding to the image wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat corresponding to the image wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
WCS catalog name: wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=12291, passed=123597
Got 123597 stars (including 111075 good ones) from the SExtractor catalog wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 123597 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
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 121489 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 121489 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 121489 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits -region wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.YwOA5xdQf6 (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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
WCS_IMAGE_NAME=wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
WCS-calibrated image found: wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
Checking if the catalog wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
WCS catalog name: wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=10176, passed=85153
Got 85153 stars (including 74898 good ones) from the SExtractor catalog wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat
util/solve_plate_with_UCAC5 got 85153 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 83709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 83708 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 83709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits -region wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.yta4TSR2KS (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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
WCS_IMAGE_NAME=wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
WCS-calibrated image found: wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
Checking if the catalog wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
WCS catalog name: wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=10176, passed=85736
Got 85736 stars (including 75493 good ones) from the SExtractor catalog wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat
util/solve_plate_with_UCAC5 got 85736 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 83405 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 83403 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 83402 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits -region wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/wcs_Peg-02-Q2b1x1_2025-12-26_19-19-08_20.00sec_-15.00C_LIGHT_0020.fits
Saving fully-calibrated image wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/wcs_Peg-02-Q2b1x1_2025-12-26_19-20-03_20.00sec_-15.00C_LIGHT_0021.fits
Saving fully-calibrated image wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-42-39_20.00sec_-4.90C_LIGHT_0750.fits
Saving fully-calibrated image wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.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_2026-04-19_CI_Peg-02-Q2b1x1_054420_TTUQ2b1x1_3409947_e4zGJ3Dk/wcs_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751.fits
Preparing the HTML report for the field Peg-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out142820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out162784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out162792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out165142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out166578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out166952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out142802.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out142845.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out166274.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out166380.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out167313.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out167833.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out142808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167522.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 226s
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: 7s
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Considering the candidate 142802_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 142802_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:02:25.97 +31:34:25.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)
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Considering the candidate 142808_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
Preparing report for the candidate 142808_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
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Considering the candidate 142817_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 142817_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:51:06.86 +30:44:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142820_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 142820_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:00:48.03 +28:51:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 0.686 1896222013870737280 330.20015629779 +28.85056150106 14.6419 14.1680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 142827_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
Preparing report for the candidate 142827_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
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Considering the candidate 142843_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 142843_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:41:24.49 +31:45:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142845_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 142845_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:52:03.28 +30:15:11.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)
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Considering the candidate 142848_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
Preparing report for the candidate 142848_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
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Considering the candidate 142850_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
Preparing report for the candidate 142850_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
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Considering the candidate 142858_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 142858_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:39:11.01 +33:48:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142861_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 142861_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:40:27.06 +33:18:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147343_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 147343_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:10:03.71 +33:08:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148678_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 148678_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:39:26.28 +30:09:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149038_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 149038_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:44:32.47 +25:36:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150591_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 150591_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:55:17.93 +30:49:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152003_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 152003_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:53:04.74 +32:44:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152294_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 152294_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:39:31.13 +31:53:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154425_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 154425_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:50:50.25 +32:41:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154437_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 154437_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:14:28.66 +33:57:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154448_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 154448_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:09:20.84 +33:11:26.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 155094_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 155094_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:48:28.78 +31:27:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155335_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 155335_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:46:48.98 +33:28:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156008_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 156008_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:44:49.21 +31:44:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156427_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 156427_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:39:55.14 +31:19:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156795_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 156795_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:09:21.18 +33:46:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157068_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 157068_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:16:18.25 +26:17:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157088_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 157088_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:39:52.47 +28:48:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157146_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 157146_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:43:28.67 +27:20:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157220_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 157220_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:43:45.32 +31:44:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157428_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 157428_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:50:24.74 +32:02:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157971_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 157971_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:52:40.86 +28:48:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158497_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 158497_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:53:48.87 +28:21:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159195_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 159195_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:09:22.66 +32:56:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159536_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 159536_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:11:11.80 +27:06:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160024_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 160024_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:00:55.53 +31:14:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160117_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 160117_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:51:07.86 +30:57:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160420_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 160420_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:59:12.91 +30:30:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160599_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 160599_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:49:53.42 +28:40:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160672_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 160672_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:04:57.89 +29:58:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160942_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 160942_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:52:21.89 +28:03:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161141_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 161141_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:54:35.90 +30:44:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161277_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
Preparing report for the candidate 161277_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161299_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 161299_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:59:42.89 +33:03:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161791_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 161791_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:48:39.01 +30:22:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161879_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 161879_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:52:32.68 +28:55:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161923_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 161923_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:51:47.98 +28:56:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162738_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 162738_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:09:25.54 +32:12:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162784_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 162784_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:40:41.62 +27:41:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 2.270 1800772589126592256 325.17327497375 +27.68940973073 14.0793 13.2636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 162792_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 162792_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:52:09.02 +33:03:00.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)
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Considering the candidate 162967_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 162967_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:51:55.31 +29:58:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163083_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 163083_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:59:42.97 +31:19:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165142_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 165142_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:54:53.58 +25:44:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 4.569 1796691820440145664 328.72302557149 +25.73921924222 14.0960 13.4064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 166161_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 166161_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:48:53.28 +30:47:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166274_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 166274_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:47:38.26 +28:15:20.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)
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Considering the candidate 166380_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 166380_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:57:35.13 +33:05:14.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)
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Considering the candidate 166578_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 166578_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:40:26.85 +33:35:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 3.947 1947160295943037440 325.11181265365 +33.59482140512 14.6430 14.1807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 166747_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
Preparing report for the candidate 166747_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
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Considering the candidate 166952_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 166952_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:40:51.04 +28:02:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 1.482 1800798668168129152 325.21290357268 +28.04636774818 14.7378 14.1682 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167038_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 167038_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:39:15.74 +33:44:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167046_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 167046_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:42:52.93 +31:29:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 1.497 1945897541194500608 325.72099711011 +31.49026774516 14.5887 13.9400 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167068_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 167068_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:41:26.99 +33:45:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167139_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 167139_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:41:15.76 +33:47:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 1.535 1947544369097354240 325.31589005543 +33.78719950725 14.4105 13.9356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167248_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 167248_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:43:01.33 +29:36:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167305_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 167305_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:48:40.89 +31:57:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167313_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 167313_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:46:13.05 +31:18:56.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)
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Considering the candidate 167475_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
Preparing report for the candidate 167475_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
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Considering the candidate 167491_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 167491_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:55:00.12 +33:42:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167522_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
Preparing report for the candidate 167522_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
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Considering the candidate 167833_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 167833_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:45:47.95 +29:38:28.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)
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Considering the candidate 167868_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 167868_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:55:57.78 +32:40:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 1.731 1898264704616630144 328.99034013679 +32.66966505986 14.4015 13.5298 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167920_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 167920_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:58:53.72 +32:31:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18422_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 18422_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:16:05.53 +33:40:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95204_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 95204_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:05:10.62 +26:14:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103383_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 103383_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:14:58.83 +26:45:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24964_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 24964_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:15:59.68 +33:11:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21359_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 21359_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:07:45.01 +33:29:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64674_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 64674_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
Rejecting candidate due to large distance (41.3") between the two second-epoch detections
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Considering the candidate 108790_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 108790_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:57:52.91 +27:20:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111999_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 111999_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:12:38.03 +28:42:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109426_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 109426_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:58:06.72 +27:23:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117742_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 117742_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 22:17:09.57 +27:51:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57093_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 57093_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
**** FOUND 21:54:03.40 +30:50:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72014_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751
The candidate 72014_fd_Peg-02-Q2b1x1_2026-04-19_05-43-31_20.00sec_-5.00C_LIGHT_0751 did not pass the final checks
