This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 04.4654 2461287.9654 12.43 21:56:09.26 +31:14:57.8
84.38591 -18.20531 galactic Peg Second-epoch detections are separated by 1.1" and 8.3 pix
The object was found in VSX 0" ASASSN-V J215609.23+311457.8
Type: L
# Max. Min./Amp. JD0 Period
13.570 V 14.160 V
The object was not found in astcheck.
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 21:56:09.26 +31:14:57.8: 13.40 +/- 0.03 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 21:56:09.26 +31:14:57.8: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
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
ASASSN-V J215609.23+311457.8,2461287.9654,12.43,0.05,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
ASASSN-V J215609.23+311457.8 20260904.4654 12.43CV 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 09 04.4654 2461287.9654 12.11 21:52:52.55 +30:33:46.8
83.35318 -18.26510 galactic Peg Second-epoch detections are separated by 0.3" and 8.4 pix
The object was found in VSX 2" NSVS J2152526+303349
Type: L:
# Max. Min./Amp. JD0 Period
10.855 R1 Y 0.404 R1 81.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 21:52:52.55 +30:33:46.8: 13.08 +/- 0.02 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 21:52:52.55 +30:33:46.8: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
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
NSVS J2152526+303349,2461287.9654,12.11,0.05,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
NSVS J2152526+303349 20260904.4654 12.11CV 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 09 04.4654 2461287.9654 11.81 21:51:55.53 +29:17:14.2
82.29936 -19.08560 galactic Peg Second-epoch detections are separated by 0.7" and 8.3 pix
The object was found in VSX 1" V0385 Peg
Type: LB
# Max. Min./Amp. JD0 Period
11.900 V 13.500 V 98.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 21:51:55.53 +29:17:14.2: 12.74 +/- 0.01 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 21:51:55.53 +29:17:14.2: 12.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0385 Peg,2461287.9654,11.81,0.05,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
V0385 Peg 20260904.4654 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.87124377 21.07.2026 08:54:25.462 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
First image: 2461242.87124377 21.07.2026 08:54:25.462 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
Last image: 2461287.96565416 04.09.2026 11:10:22.519 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.37
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 15171
Objects passed selection criteria: 15101
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 10666.5
Average stars matched: 10387.8 (97.3867 %)
Memory usage VmPeak: 242460 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Sep 4 06:12:38 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.87124377 21.07.2026 08:54:25.462 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
First image: 2461242.87124377 21.07.2026 08:54:25.462 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
Last image: 2461287.96565416 04.09.2026 11:10:22.519 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 50
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.03
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: 23 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 106538
Objects passed selection criteria: 106242
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 77635.2
Average stars matched: 74663.8 (96.1725 %)
Memory usage VmPeak: 511904 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Sep 4 06:13:36 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
SExtractor catalog cache: saved Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.cat to cache
SExtractor catalog cache: saved Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.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_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.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: 2461287.96506799
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_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits exists and is non-empty
wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits exists and is non-empty
wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits exists and is non-empty
wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits (1st reference image)
verification OK: wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:00:01.064 +29:59:49.72 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits (1st new image)
verification OK: wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
Image size: 937.6'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:00:04.663 +30:00:06.94 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:00:01.064 +29:59:49.72
Second-epoch image center 22:00:04.663 +30:00:06.94
Angular distance between the image centers 0.0138 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits (2nd new image)
verification OK: wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
Image size: 937.6'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:00:01.624 +29:59:36.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:00:01.064 +29:59:49.72
Second-epoch image center 22:00:01.624 +29:59:36.10
Angular distance between the image centers 0.0043 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 22:00:04.663 +30:00:06.94
Second-epoch second image center 22:00:01.624 +29:59:36.10
Angular distance between the image centers 0.01392 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits &> /tmp/tmp.ek3v70LNBb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits &> /tmp/tmp.zAnNUk1PMA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits &> /tmp/tmp.DSsuxseA3z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits &> /tmp/tmp.YaxVRqrBNt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.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_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits and wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits and wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat
Found non-empty wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits and wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat
The reference image (wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits) and catalog (wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat) found
'wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat' -> 'wcsmag.cat'
Read 22512 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 320.4888 to 339.4674 deg, Dec +24.5257 to +35.2598 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 320.4888 to 339.4674 deg, Dec 24.5257 to 35.2598 deg
Loaded 15127 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): 11287 out of 12041 total matches.
Matched with Tycho-2 12041 out of 22512 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.697200
a=0.000000 b=1.000000 c=22.697200
From vast_summary.log: estimated ref. image limiting mag.: -7.37
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.33
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.33
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 22512 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 320.4888 to 339.4674 deg, Dec +24.5257 to +35.2598 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 320.4888 to 339.4674 deg, Dec 24.5257 to 35.2598 deg
Loaded 15127 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): 11287 out of 12041 total matches.
Matched with Tycho-2 12041 out of 22512 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
Forced-photometry filter: calibrated wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits -> calib.txt_param_ref_wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits (aperture=6.1)
Read 22616 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 320.4892 to 339.4657 deg, Dec +24.5269 to +35.2573 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 320.4892 to 339.4657 deg, Dec 24.5269 to 35.2573 deg
Loaded 15118 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): 11237 out of 12022 total matches.
Matched with Tycho-2 12022 out of 22616 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
Forced-photometry filter: calibrated wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits -> calib.txt_param_ref_wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
2.2 pix Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
2.5 pix fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
2.5 pix fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
Limiting magnitude estimates:
15.3 mag. Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
15.4 mag. Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
13.8 mag. fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
13.8 mag. fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.ek3v70LNBb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.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_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits' -> 'wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
WCS_IMAGE_NAME=wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
WCS-calibrated image found: wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
Checking if the catalog wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat corresponding to the image wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits alredy exist and is non-empty...
Catalog wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat corresponding to the image wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.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_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
WCS catalog name: wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1649, bad_region=6203, passed=22512
Got 22512 stars (including 15069 good ones) from the SExtractor catalog wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat
util/solve_plate_with_UCAC5 got 22512 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 4930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 17500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 17500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 17500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4930 stars left (next iteration limit 5423)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits N_match=4930 sigma_overall_arcsec=0.385 sigma_q1_arcsec=0.334 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.411 sigma_q4_arcsec=0.389 n_q1=1610 n_q2=1027 n_q3=1344 n_q4=949 worst_quadrant_to_overall_ratio=1.115
The image catalog is written to wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits -region wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.zAnNUk1PMA (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.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_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits' -> 'wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
WCS_IMAGE_NAME=wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
WCS-calibrated image found: wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
Checking if the catalog wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat corresponding to the image wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits alredy exist and is non-empty...
Catalog wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat corresponding to the image wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.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_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
WCS catalog name: wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1699, bad_region=6303, passed=22616
Got 22616 stars (including 15027 good ones) from the SExtractor catalog wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat
util/solve_plate_with_UCAC5 got 22616 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4928 matched stars entering correct_measured_positions(), 4928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4928 matched stars entering correct_measured_positions(), 17525 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4928 matched stars entering correct_measured_positions(), 17525 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4928 matched stars entering correct_measured_positions(), 17525 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4928 stars left (next iteration limit 5420)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits N_match=4928 sigma_overall_arcsec=0.434 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.480 sigma_q3_arcsec=0.438 sigma_q4_arcsec=0.429 n_q1=1608 n_q2=1025 n_q3=1346 n_q4=949 worst_quadrant_to_overall_ratio=1.108
The image catalog is written to wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits -region wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.DSsuxseA3z (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_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.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_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
WCS_IMAGE_NAME=wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
WCS-calibrated image found: wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
Checking if the catalog wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.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_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
WCS catalog name: wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=371, bad_region=1509, passed=6918
Got 6918 stars (including 5154 good ones) from the SExtractor catalog wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat
util/solve_plate_with_UCAC5 got 6918 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4913 matched stars entering correct_measured_positions(), 4913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4913 matched stars entering correct_measured_positions(), 5776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 5776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 5776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4912 stars left (next iteration limit 5404)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4912 robust_rms=6.382 arcsec worst_quadrant_rms=6.963 arcsec
SIP_REFIT: SIP order 3 trial: matched=4912 robust_rms=0.475 arcsec worst_quadrant_rms=0.521 arcsec
SIP_REFIT: SIP order 5 trial: matched=4912 robust_rms=0.445 arcsec worst_quadrant_rms=0.483 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4912 robust_rms_before=0.658 arcsec robust_rms_before_corrected=0.437 arcsec robust_rms_after=0.445 arcsec worst_quadrant_rms_before=0.493 worst_quadrant_rms_after=0.483
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.493 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits N_match=4912 sigma_overall_arcsec=0.447 sigma_q1_arcsec=0.449 sigma_q2_arcsec=0.485 sigma_q3_arcsec=0.413 sigma_q4_arcsec=0.454 n_q1=1301 n_q2=1144 n_q3=1482 n_q4=985 worst_quadrant_to_overall_ratio=1.086
The image catalog is written to wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits -region wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.YaxVRqrBNt (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_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.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_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
WCS_IMAGE_NAME=wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
WCS-calibrated image found: wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
Checking if the catalog wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.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_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
WCS catalog name: wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=373, bad_region=1496, passed=6361
Got 6361 stars (including 4641 good ones) from the SExtractor catalog wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat
util/solve_plate_with_UCAC5 got 6361 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4582 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4564 matched stars entering correct_measured_positions(), 4563 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4564 matched stars entering correct_measured_positions(), 5220 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4583 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4563 matched stars entering correct_measured_positions(), 5220 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 4563 matched stars entering correct_measured_positions(), 5220 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4563 stars left (next iteration limit 5020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4563 robust_rms=6.191 arcsec worst_quadrant_rms=6.964 arcsec
SIP_REFIT: SIP order 3 trial: matched=4563 robust_rms=0.508 arcsec worst_quadrant_rms=0.542 arcsec
SIP_REFIT: SIP order 5 trial: matched=4563 robust_rms=0.470 arcsec worst_quadrant_rms=0.523 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=4563 robust_rms_before=0.677 arcsec robust_rms_before_corrected=0.446 arcsec robust_rms_after=0.508 arcsec worst_quadrant_rms_before=0.527 worst_quadrant_rms_after=0.542
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.527 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits N_match=4563 sigma_overall_arcsec=0.455 sigma_q1_arcsec=0.445 sigma_q2_arcsec=0.518 sigma_q3_arcsec=0.425 sigma_q4_arcsec=0.469 n_q1=998 n_q2=1145 n_q3=1417 n_q4=1003 worst_quadrant_to_overall_ratio=1.139
The image catalog is written to wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits -region wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits to local_wcs_cache/
'wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits' -> 'local_wcs_cache/wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits'
Saving the final (post-refit) wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits to local_wcs_cache/
'wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits' -> 'local_wcs_cache/wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits'
Saving the final (post-refit) wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits to local_wcs_cache/
'wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits' -> 'local_wcs_cache/wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits'
Saving the final (post-refit) wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits to local_wcs_cache/
'wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits' -> 'local_wcs_cache/wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits sigma_overall=0.385 worst_q_ratio=1.115
ref2=Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits sigma_overall=0.434 worst_q_ratio=1.108
new1=fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits sigma_overall=0.447 worst_q_ratio=1.086
new2=fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits sigma_overall=0.455 worst_q_ratio=1.139
reference average sigma_overall=0.4095 worst_q_ratio=1.1115
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923_astrometric_residuals.png (4930 matched stars from wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924_astrometric_residuals.png (4928 matched stars from wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738_astrometric_residuals.png (4912 matched stars from wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739_astrometric_residuals.png (4563 matched stars from wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits'
Saving fully-calibrated image wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits'
Preparing the HTML report for the field Peg-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 22:08:34.74 +33:06:24.9: 10.49 +/- 0.00 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 22:08:34.74 +33:06:24.9: 10.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.51 +/- 0.00
Forced photometry filter REJECTED candidate at 22:08:34.74 +33:06:24.9: ref_mag=10.51 +/- 0.00 new_mean_mag=10.8334 delta=-0.33 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31082_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 31082_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31103_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 31103_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 21:42:57.10 +31:27:30.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03613_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 03613_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 21:43:31.62 +33:48:47.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
SExtractor catalog cache: saved Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.cat to cache
SExtractor catalog cache: saved Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.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_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
Creating symlink local_wcs_cache/wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits exists and is non-empty
wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits exists and is non-empty
wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits exists and is non-empty
wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits (1st reference image)
verification OK: wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:00:01.064 +29:59:49.72 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits (1st new image)
verification OK: wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
Image size: 937.6'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:00:04.663 +30:00:06.94 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 22:00:01.064 +29:59:49.72
Second-epoch image center 22:00:04.663 +30:00:06.94
Angular distance between the image centers 0.0138 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits (2nd new image)
verification OK: wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
Image size: 937.6'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 22:00:01.624 +29:59:36.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:00:01.064 +29:59:49.72
Second-epoch image center 22:00:01.624 +29:59:36.10
Angular distance between the image centers 0.0043 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 22:00:04.663 +30:00:06.94
Second-epoch second image center 22:00:01.624 +29:59:36.10
Angular distance between the image centers 0.01392 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits &> /tmp/tmp.sJPEc4TFQC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits &> /tmp/tmp.LkL46nkBCM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits &> /tmp/tmp.tB4bqIsBit
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits &> /tmp/tmp.toDbyc2v1E
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.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_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits and wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits and wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat
Found non-empty wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits and wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat
The reference image (wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits) and catalog (wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat) found
'wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat' -> 'wcsmag.cat'
Read 147872 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 320.4888 to 339.5207 deg, Dec +24.5096 to +35.2617 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 320.4888 to 339.5207 deg, Dec 24.5096 to 35.2617 deg
Loaded 15193 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): 9704 out of 12253 total matches.
Matched with Tycho-2 12253 out of 147872 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.558600
a=0.000000 b=1.000000 c=22.558600
From vast_summary.log: estimated ref. image limiting mag.: -7.03
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.53
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 147872 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 320.4888 to 339.5207 deg, Dec +24.5096 to +35.2617 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 320.4888 to 339.5207 deg, Dec 24.5096 to 35.2617 deg
Loaded 15193 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): 9704 out of 12253 total matches.
Matched with Tycho-2 12253 out of 147872 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
Forced-photometry filter: calibrated wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits -> calib.txt_param_ref_wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits (aperture=4.6)
Read 150494 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 320.4859 to 339.5164 deg, Dec +24.4971 to +35.2574 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 320.4859 to 339.5164 deg, Dec 24.4971 to 35.2574 deg
Loaded 15198 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): 9598 out of 12224 total matches.
Matched with Tycho-2 12224 out of 150494 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
Forced-photometry filter: calibrated wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits -> calib.txt_param_ref_wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 42 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
2.1 pix Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
2.4 pix fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
2.4 pix fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
Limiting magnitude estimates:
15.5 mag. Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
15.5 mag. Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
14.0 mag. fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
13.9 mag. fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.sJPEc4TFQC (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.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_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits' -> 'wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
WCS_IMAGE_NAME=wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
WCS-calibrated image found: wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
Checking if the catalog wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat corresponding to the image wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits alredy exist and is non-empty...
Catalog wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat corresponding to the image wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.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_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits
WCS catalog name: wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=32, blended=14956, bad_region=31760, passed=147840
Got 147840 stars (including 104581 good ones) from the SExtractor catalog wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat
util/solve_plate_with_UCAC5 got 147840 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 4930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 123762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 123762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 123762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4930 stars left (next iteration limit 5423)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits N_match=4930 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.341 sigma_q2_arcsec=0.427 sigma_q3_arcsec=0.400 sigma_q4_arcsec=0.370 n_q1=1670 n_q2=984 n_q3=1349 n_q4=927 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits -region wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.LkL46nkBCM (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.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_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits' -> 'wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
WCS_IMAGE_NAME=wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
WCS-calibrated image found: wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
Checking if the catalog wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat corresponding to the image wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits alredy exist and is non-empty...
Catalog wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat corresponding to the image wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.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_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits
WCS catalog name: wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=15301, bad_region=32065, passed=150463
Got 150463 stars (including 106603 good ones) from the SExtractor catalog wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat
util/solve_plate_with_UCAC5 got 150463 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4928 matched stars entering correct_measured_positions(), 4928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4928 matched stars entering correct_measured_positions(), 126148 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4928 matched stars entering correct_measured_positions(), 126148 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4928 matched stars entering correct_measured_positions(), 126148 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4928 stars left (next iteration limit 5420)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits N_match=4928 sigma_overall_arcsec=0.419 sigma_q1_arcsec=0.379 sigma_q2_arcsec=0.462 sigma_q3_arcsec=0.434 sigma_q4_arcsec=0.410 n_q1=1653 n_q2=989 n_q3=1365 n_q4=921 worst_quadrant_to_overall_ratio=1.101
The image catalog is written to wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits -region wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.tB4bqIsBit (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_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.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_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
WCS_IMAGE_NAME=wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
WCS-calibrated image found: wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
Checking if the catalog wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.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_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
WCS catalog name: wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=3068, bad_region=7629, passed=48010
Got 48010 stars (including 38530 good ones) from the SExtractor catalog wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat
util/solve_plate_with_UCAC5 got 48010 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 4916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 42347 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 42347 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 4916 matched stars entering correct_measured_positions(), 42347 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4916 stars left (next iteration limit 5407)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4916 robust_rms=6.256 arcsec worst_quadrant_rms=7.321 arcsec
SIP_REFIT: SIP order 3 trial: matched=4916 robust_rms=0.472 arcsec worst_quadrant_rms=0.502 arcsec
SIP_REFIT: SIP order 5 trial: matched=4916 robust_rms=0.441 arcsec worst_quadrant_rms=0.466 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4916 robust_rms_before=0.662 arcsec robust_rms_before_corrected=0.432 arcsec robust_rms_after=0.441 arcsec worst_quadrant_rms_before=0.468 worst_quadrant_rms_after=0.466
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.468 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits N_match=4916 sigma_overall_arcsec=0.439 sigma_q1_arcsec=0.452 sigma_q2_arcsec=0.471 sigma_q3_arcsec=0.414 sigma_q4_arcsec=0.450 n_q1=1328 n_q2=1044 n_q3=1603 n_q4=941 worst_quadrant_to_overall_ratio=1.073
The image catalog is written to wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits -region wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.toDbyc2v1E (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_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.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_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
WCS_IMAGE_NAME=wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
WCS-calibrated image found: wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
Checking if the catalog wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat corresponding to the image wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.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_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
WCS catalog name: wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2801, bad_region=7543, passed=44915
Got 44915 stars (including 35771 good ones) from the SExtractor catalog wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat
util/solve_plate_with_UCAC5 got 44915 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 4922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4922 matched stars entering correct_measured_positions(), 39346 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 4935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 39346 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 39353 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4923 stars left (next iteration limit 5414)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4923 robust_rms=6.330 arcsec worst_quadrant_rms=6.510 arcsec
SIP_REFIT: SIP order 3 trial: matched=4923 robust_rms=0.505 arcsec worst_quadrant_rms=0.535 arcsec
SIP_REFIT: SIP order 5 trial: matched=4923 robust_rms=0.469 arcsec worst_quadrant_rms=0.503 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4923 robust_rms_before=0.679 arcsec robust_rms_before_corrected=0.441 arcsec robust_rms_after=0.469 arcsec worst_quadrant_rms_before=0.503 worst_quadrant_rms_after=0.503
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.503 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits N_match=4923 sigma_overall_arcsec=0.448 sigma_q1_arcsec=0.427 sigma_q2_arcsec=0.497 sigma_q3_arcsec=0.421 sigma_q4_arcsec=0.455 n_q1=1143 n_q2=1118 n_q3=1660 n_q4=1002 worst_quadrant_to_overall_ratio=1.110
The image catalog is written to wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits -region wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.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_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-09-31_20.00sec_-0.00C_LIGHT_0738.fits
Saving fully-calibrated image wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.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_2026-09-04_CI_Peg-02-Q2b1x1_061055_TTUQ2b1x1_732638_7lIMbNBI/wcs_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739.fits
Preparing the HTML report for the field Peg-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 22:18:32.77 +32:45:55.8: 12.79 +/- 0.02 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 21:58:30.03 +26:00:12.2: 12.94 +/- 0.02 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 22:09:06.55 +28:12:15.8: 11.66 +/- 0.01 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 22:16:05.25 +28:32:00.6: 13.82 +/- 0.05 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 22:25:57.15 +26:35:51.8: 12.82 +/- 0.02 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 21:56:05.65 +33:22:16.6: 12.76 +/- 0.02 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 22:07:46.74 +28:08:24.6: 13.05 +/- 0.02 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 22:18:32.77 +32:45:55.8: 12.83 +/- 0.02 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 22:16:05.25 +28:32:00.6: 13.91 +/- 0.05 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 21:58:30.03 +26:00:12.2: 12.99 +/- 0.02 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 22:25:57.15 +26:35:51.8: 12.74 +/- 0.02 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 22:09:06.55 +28:12:15.8: 11.67 +/- 0.01 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 21:56:05.65 +33:22:16.6: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter REJECTED candidate at 22:18:32.77 +32:45:55.8: ref_mag=12.81 +/- 0.01 new_mean_mag=12.8063 delta=0.00 (need > 0.90)
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Forced photometry filter REJECTED candidate at 22:16:05.25 +28:32:00.6: ref_mag=13.86 +/- 0.03 new_mean_mag=13.6299 delta=0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:58:30.03 +26:00:12.2: ref_mag=12.97 +/- 0.02 new_mean_mag=12.8101 delta=0.16 (need > 0.90)
Forced photometry reference-image weighted average: 11.66 +/- 0.01
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry filter REJECTED candidate at 22:25:57.15 +26:35:51.8: ref_mag=12.78 +/- 0.02 new_mean_mag=12.6698 delta=0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:09:06.55 +28:12:15.8: ref_mag=11.66 +/- 0.01 new_mean_mag=11.6968 delta=-0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 21:56:05.65 +33:22:16.6: ref_mag=12.78 +/- 0.01 new_mean_mag=12.4571 delta=0.32 (need > 0.90)
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 21:48:27.76 +32:46:55.4: 13.16 +/- 0.03 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 22:10:42.35 +29:18:23.5: 13.57 +/- 0.03 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 22:07:46.74 +28:08:24.6: 13.05 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Forced photometry filter REJECTED candidate at 22:07:46.74 +28:08:24.6: ref_mag=13.05 +/- 0.02 new_mean_mag=12.9359 delta=0.11 (need > 0.90)
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 21:46:32.31 +26:44:24.6: 13.03 +/- 0.03 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 21:48:27.76 +32:46:55.4: 13.14 +/- 0.03 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 22:10:42.35 +29:18:23.5: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry reference-image weighted average: 13.56 +/- 0.02
Forced photometry filter REJECTED candidate at 21:48:27.76 +32:46:55.4: ref_mag=13.15 +/- 0.02 new_mean_mag=12.9103 delta=0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:10:42.35 +29:18:23.5: ref_mag=13.56 +/- 0.02 new_mean_mag=13.1702 delta=0.39 (need > 0.90)
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 22:26:39.07 +27:45:17.1: 13.60 +/- 0.04 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 21:43:55.86 +27:49:44.5: 12.94 +/- 0.02 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 21:46:32.31 +26:44:24.6: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter REJECTED candidate at 21:46:32.31 +26:44:24.6: ref_mag=13.02 +/- 0.02 new_mean_mag=13.0577 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 22:02:41.23 +27:40:47.4: 13.49 +/- 0.04 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 21:43:55.86 +27:49:44.5: 12.98 +/- 0.02 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 22:26:39.07 +27:45:17.1: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Forced photometry filter REJECTED candidate at 21:43:55.86 +27:49:44.5: ref_mag=12.96 +/- 0.02 new_mean_mag=13.0299 delta=-0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 22:26:39.07 +27:45:17.1: ref_mag=13.55 +/- 0.03 new_mean_mag=13.4595 delta=0.09 (need > 0.90)
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 22:10:19.03 +28:09:41.9: 14.02 +/- 0.06 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 22:02:41.23 +27:40:47.4: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Forced photometry filter REJECTED candidate at 22:02:41.23 +27:40:47.4: ref_mag=13.48 +/- 0.03 new_mean_mag=13.3114 delta=0.17 (need > 0.90)
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 21:56:09.26 +31:14:57.8: 13.40 +/- 0.03 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 22:10:19.03 +28:09:41.9: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.04
Forced photometry filter REJECTED candidate at 22:10:19.03 +28:09:41.9: ref_mag=13.98 +/- 0.04 new_mean_mag=13.5738 delta=0.41 (need > 0.90)
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 21:52:52.55 +30:33:46.8: 13.08 +/- 0.02 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 21:56:09.26 +31:14:57.8: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Forced photometry filter KEPT candidate at 21:56:09.26 +31:14:57.8: ref_mag=13.37 +/- 0.02 new_mean_mag=12.4268 delta=0.95 (need > 0.90)
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-54-25_20.00sec_5.00C_LIGHT_0923.fits at 21:51:55.53 +29:17:14.2: 12.74 +/- 0.01 detection
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 21:52:52.55 +30:33:46.8: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 21:52:52.55 +30:33:46.8: ref_mag=13.07 +/- 0.02 new_mean_mag=12.1086 delta=0.97 (need > 0.90)
Forced photometry on wcs_Peg-02-Q2b1x1_2026-07-21_03-55-31_20.00sec_5.00C_LIGHT_0924.fits at 21:51:55.53 +29:17:14.2: 12.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Forced photometry filter KEPT candidate at 21:51:55.53 +29:17:14.2: ref_mag=12.74 +/- 0.01 new_mean_mag=11.8078 delta=0.93 (need > 0.90)
Adding exclusion_list_local.txt__out60403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90180.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 169370_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169370_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
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Considering the candidate 169373_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169373_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:13:40.51 +29:32:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169378_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169378_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 21:46:38.39 +26:44:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169416_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169416_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
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Considering the candidate 169433_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169433_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:10:03.72 +33:08:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169452_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169452_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
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Considering the candidate 169458_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169458_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:15:37.00 +25:46:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169468_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169468_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
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Considering the candidate 169478_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169478_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
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Considering the candidate 169480_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169480_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
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Considering the candidate 169493_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169493_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:16:18.19 +26:17:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169496_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169496_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:06:49.71 +25:51:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169497_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169497_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
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Considering the candidate 169502_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169502_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:10:30.05 +30:47:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169507_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169507_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:01:00.01 +31:31:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169521_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169521_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
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Considering the candidate 169522_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169522_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
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Considering the candidate 169524_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169524_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
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Considering the candidate 169528_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169528_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:21:21.55 +28:17:57.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 169529_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169529_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
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Considering the candidate 169538_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169538_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:12:46.44 +26:54:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169540_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169540_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 21:44:28.07 +26:18:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169551_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169551_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:31:38.72 +29:31:53.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 169553_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169553_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
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Considering the candidate 169559_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169559_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:02:45.83 +27:41:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169560_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169560_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:31:39.50 +29:33:07.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 169563_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169563_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:11:11.75 +27:06:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169565_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169565_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
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Considering the candidate 169572_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169572_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:07:22.85 +27:42:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169585_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169585_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 21:54:51.76 +29:20:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169599_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169599_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
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Considering the candidate 169607_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 169607_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:13:44.10 +30:35:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66604_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 66604_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 21:54:03.48 +30:50:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27863_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 27863_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:00:44.00 +33:23:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60403_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
Preparing report for the candidate 60403_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
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Considering the candidate 120379_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 120379_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 22:14:59.05 +26:45:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71078_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
Preparing report for the candidate 71078_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
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Considering the candidate 56524_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 56524_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 21:42:57.14 +31:27:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81030_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 81030_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
Rejecting candidate due to large distance (50.0") between the two second-epoch detections
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Considering the candidate 90180_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
Preparing report for the candidate 90180_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
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Considering the candidate 20290_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 20290_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks
**** FOUND 21:43:31.62 +33:48:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37294_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739
The candidate 37294_fd_Peg-02-Q2b1x1_2026-09-04_06-10-22_20.00sec_0.00C_LIGHT_0739 did not pass the final checks