This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN
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 07 29.4577 2461250.9577 11.00 23:15:25.40 +10:56:59.4
88.28896 -45.36571 galactic Peg Second-epoch detections are separated by 0.7" and 9.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.198 Ampella -1 -0 1 11.3 0 0
Forced photometry on wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:15:25.40 +10:56:59.4: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:15:25.40 +10:56:59.4: 15.66 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461250.9577,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260729.4577 11.00CV 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 07 29.4577 2461250.9577 11.94 23:02:38.09 +11:14:15.1
84.80379 -43.43472 galactic Peg Second-epoch detections are separated by 0.7" and 9.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.690 Wratislavia -0 -0 0 12.5 0 0
Forced photometry on wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:38.09 +11:14:15.1: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:38.09 +11:14:15.1: 15.72 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461250.9577,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260729.4577 11.94CV 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: 2461203.92142735 12.06.2026 10:06:41.323 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
First image: 2461203.92142735 12.06.2026 10:06:41.323 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Last image: 2461250.95798244 29.07.2026 10:59:19.683 /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5793
Objects passed selection criteria: 5785
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 3757.5
Average stars matched: 3476.75 (92.5283 %)
Memory usage VmPeak: 232632 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jul 28 18:39:20 CDT 2026
VaST build number 1.0rc89-184-g1e68672b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-28)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jul 29 06:04:37 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: 2461203.92142735 12.06.2026 10:06:41.323 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
First image: 2461203.92142735 12.06.2026 10:06:41.323 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Last image: 2461250.95798244 29.07.2026 10:59:19.683 /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 15 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
Total objects detected (at least 2 times): 35155
Objects passed selection criteria: 35065
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 23842.8
Average stars matched: 22391.8 (93.9143 %)
Memory usage VmPeak: 259544 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jul 28 18:39:20 CDT 2026
VaST build number 1.0rc89-184-g1e68672b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-28)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jul 29 06:07:38 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-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
SExtractor catalog cache: saved Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.cat to cache
SExtractor catalog cache: saved Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.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: 2461250.95748451
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-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits exists and is non-empty
Saving wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits to local_wcs_cache/
'wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits' -> 'local_wcs_cache/wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits'
wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits exists and is non-empty
Saving wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits to local_wcs_cache/
'wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits' -> 'local_wcs_cache/wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits'
wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits exists and is non-empty
Saving wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits to local_wcs_cache/
'wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits' -> 'local_wcs_cache/wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits'
wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits exists and is non-empty
Saving wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits to local_wcs_cache/
'wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits' -> 'local_wcs_cache/wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits (1st reference image)
verification OK: wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:38.452 +14:00:51.18 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits (1st new image)
verification OK: wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
Image size: 936.9'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: 23:06:41.411 +14:00:09.51 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:06:38.452 +14:00:51.18
Second-epoch image center 23:06:41.411 +14:00:09.51
Angular distance between the image centers 0.0166 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits (2nd new image)
verification OK: wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
Image size: 936.9'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: 23:06:43.446 +14:00:55.70 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:06:38.452 +14:00:51.18
Second-epoch image center 23:06:43.446 +14:00:55.70
Angular distance between the image centers 0.0202 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:06:41.411 +14:00:09.51
Second-epoch second image center 23:06:43.446 +14:00:55.70
Angular distance between the image centers 0.01524 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits &> /tmp/tmp.r4NrSeGExq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits &> /tmp/tmp.gWqyaA9KvQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits &> /tmp/tmp.a1DOTfbkUG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits &> /tmp/tmp.TMPPHNMqUl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits and wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits and wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
Found non-empty wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits and wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
The reference image (wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits) and catalog (wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat) found
'wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat' -> 'wcsmag.cat'
Read 7458 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.3587 to 354.8627 deg, Dec +8.6419 to +19.2809 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 338.3587 to 354.8627 deg, Dec 8.6419 to 19.2809 deg
Loaded 5970 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): 4723 out of 4851 total matches.
Matched with Tycho-2 4851 out of 7458 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.608100
a=0.000000 b=1.000000 c=22.608100
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.99
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.99
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7458 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.3587 to 354.8627 deg, Dec +8.6419 to +19.2809 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 338.3587 to 354.8627 deg, Dec 8.6419 to 19.2809 deg
Loaded 5970 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): 4723 out of 4851 total matches.
Matched with Tycho-2 4851 out of 7458 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits:
Forced-photometry filter: calibrated wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits -> calib.txt_param_ref_wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits (aperture=6.2)
Read 7660 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4285 to 355.2030 deg, Dec +8.2117 to +19.5193 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 338.4285 to 355.2030 deg, Dec 8.2117 to 19.5193 deg
Loaded 6456 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): 4837 out of 4961 total matches.
Matched with Tycho-2 4961 out of 7660 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits:
Forced-photometry filter: calibrated wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits -> calib.txt_param_ref_wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
2.5 pix Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
2.5 pix fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
2.5 pix fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
2.3 pix wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
2.5 pix wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
Limiting magnitude estimates:
15.0 mag. Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
14.9 mag. Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
13.1 mag. fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
13.1 mag. fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 10.5 (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
############ /tmp/tmp.r4NrSeGExq (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_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits' -> 'wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
WCS-calibrated image found: wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Checking if the catalog wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
WCS catalog name: wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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=405, bad_region=1639, passed=7458
Got 7458 stars (including 5478 good ones) from the SExtractor catalog wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
util/solve_plate_with_UCAC5 got 7458 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 4850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 6114 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4851 matched stars entering correct_measured_positions(), 6114 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4851 matched stars entering correct_measured_positions(), 6114 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4851 stars left (next iteration limit 5335)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits N_match=4851 sigma_overall_arcsec=0.387 sigma_q1_arcsec=0.354 sigma_q2_arcsec=0.351 sigma_q3_arcsec=0.429 sigma_q4_arcsec=0.380 n_q1=1469 n_q2=869 n_q3=1670 n_q4=843 worst_quadrant_to_overall_ratio=1.109
The image catalog is written to wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits -region wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.gWqyaA9KvQ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits' -> 'wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
WCS-calibrated image found: wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
Checking if the catalog wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
WCS catalog name: wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.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=367, bad_region=1472, passed=7660
Got 7660 stars (including 5882 good ones) from the SExtractor catalog wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat
util/solve_plate_with_UCAC5 got 7660 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 4852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 6445 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 6445 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 6445 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Excluding outliers - 4852 stars left (next iteration limit 5337)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits N_match=4852 sigma_overall_arcsec=0.237 sigma_q1_arcsec=0.252 sigma_q2_arcsec=0.229 sigma_q3_arcsec=0.234 sigma_q4_arcsec=0.200 n_q1=1497 n_q2=811 n_q3=1729 n_q4=815 worst_quadrant_to_overall_ratio=1.067
The image catalog is written to wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits -region wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.a1DOTfbkUG (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_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.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_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
Checking if the catalog wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
WCS catalog name: wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.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=175, bad_region=501, passed=2084
Got 2084 stars (including 1450 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat
util/solve_plate_with_UCAC5 got 2084 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 1420 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1416 matched stars entering correct_measured_positions(), 1416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1416 matched stars entering correct_measured_positions(), 1670 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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 1420 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1416 matched stars entering correct_measured_positions(), 1670 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 1416 matched stars entering correct_measured_positions(), 1670 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 1416 stars left (next iteration limit 1557)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1416 robust_rms=6.998 arcsec worst_quadrant_rms=9.001 arcsec
SIP_REFIT: SIP order 3 trial: matched=1416 robust_rms=0.409 arcsec worst_quadrant_rms=0.442 arcsec
SIP_REFIT: SIP order 5 trial: matched=1416 robust_rms=0.369 arcsec worst_quadrant_rms=0.420 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=1416 robust_rms_before=0.816 arcsec robust_rms_before_corrected=0.383 arcsec robust_rms_after=0.409 arcsec worst_quadrant_rms_before=0.453 worst_quadrant_rms_after=0.442
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.453 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits N_match=1416 sigma_overall_arcsec=0.393 sigma_q1_arcsec=0.363 sigma_q2_arcsec=0.467 sigma_q3_arcsec=0.334 sigma_q4_arcsec=0.482 n_q1=419 n_q2=278 n_q3=439 n_q4=280 worst_quadrant_to_overall_ratio=1.228
The image catalog is written to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits -region wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.TMPPHNMqUl (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_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.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_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
Checking if the catalog wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
WCS catalog name: wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.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=176, bad_region=510, passed=2036
Got 2036 stars (including 1398 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat
util/solve_plate_with_UCAC5 got 2036 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 1367 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1364 matched stars entering correct_measured_positions(), 1364 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1364 matched stars entering correct_measured_positions(), 1613 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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 1367 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1364 matched stars entering correct_measured_positions(), 1613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 1364 matched stars entering correct_measured_positions(), 1613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 1364 stars left (next iteration limit 1500)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1364 robust_rms=7.134 arcsec worst_quadrant_rms=9.466 arcsec
SIP_REFIT: SIP order 3 trial: matched=1364 robust_rms=0.409 arcsec worst_quadrant_rms=0.430 arcsec
SIP_REFIT: SIP order 5 trial: matched=1364 robust_rms=0.378 arcsec worst_quadrant_rms=0.427 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=1364 robust_rms_before=0.835 arcsec robust_rms_before_corrected=0.401 arcsec robust_rms_after=0.409 arcsec worst_quadrant_rms_before=0.476 worst_quadrant_rms_after=0.430
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.476 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits N_match=1364 sigma_overall_arcsec=0.417 sigma_q1_arcsec=0.383 sigma_q2_arcsec=0.455 sigma_q3_arcsec=0.395 sigma_q4_arcsec=0.478 n_q1=408 n_q2=272 n_q3=418 n_q4=266 worst_quadrant_to_overall_ratio=1.148
The image catalog is written to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits -region wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits sigma_overall=0.387 worst_q_ratio=1.109
ref2=Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits sigma_overall=0.237 worst_q_ratio=1.067
new1=fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits sigma_overall=0.393 worst_q_ratio=1.228
new2=fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits sigma_overall=0.417 worst_q_ratio=1.148
reference average sigma_overall=0.312 worst_q_ratio=1.088
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287_astrometric_residuals.png (4851 matched stars from wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366_astrometric_residuals.png (4852 matched stars from wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.21 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012_astrometric_residuals.png (1416 matched stars from wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013_astrometric_residuals.png (1364 matched stars from wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits'
Saving fully-calibrated image wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits'
Preparing the HTML report for the field Peg-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01178_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013
The candidate 01178_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013 did not pass the final checks
**** FOUND 23:06:39.32 +10:32:40.2 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-10-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-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
SExtractor catalog cache: saved Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.cat to cache
SExtractor catalog cache: saved Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Creating symlink local_wcs_cache/wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits exists and is non-empty
wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits exists and is non-empty
wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits exists and is non-empty
wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits (1st reference image)
verification OK: wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:06:38.452 +14:00:51.18 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits (1st new image)
verification OK: wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
Image size: 936.9'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: 23:06:41.411 +14:00:09.51 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:06:38.452 +14:00:51.18
Second-epoch image center 23:06:41.411 +14:00:09.51
Angular distance between the image centers 0.0166 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits (2nd new image)
verification OK: wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
Image size: 936.9'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: 23:06:43.446 +14:00:55.70 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:06:38.452 +14:00:51.18
Second-epoch image center 23:06:43.446 +14:00:55.70
Angular distance between the image centers 0.0202 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 23:06:41.411 +14:00:09.51
Second-epoch second image center 23:06:43.446 +14:00:55.70
Angular distance between the image centers 0.01524 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits &> /tmp/tmp.htIn9sbr14
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits &> /tmp/tmp.drB9s3y7eP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits &> /tmp/tmp.8DfIXRY333
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits &> /tmp/tmp.FUY5PxxD1W
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits and wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits and wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
Found non-empty wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits and wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
The reference image (wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits) and catalog (wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat) found
'wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat' -> 'wcsmag.cat'
Read 44707 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.3587 to 354.8627 deg, Dec +8.6411 to +19.2831 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 338.3587 to 354.8627 deg, Dec 8.6411 to 19.2831 deg
Loaded 5972 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4687 out of 5110 total matches.
Matched with Tycho-2 5110 out of 44707 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.475500
a=0.000000 b=1.000000 c=22.475500
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 44707 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.3587 to 354.8627 deg, Dec +8.6411 to +19.2831 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 338.3587 to 354.8627 deg, Dec 8.6411 to 19.2831 deg
Loaded 5972 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4687 out of 5110 total matches.
Matched with Tycho-2 5110 out of 44707 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits:
Forced-photometry filter: calibrated wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits -> calib.txt_param_ref_wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits (aperture=4.8)
Read 42031 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 338.4279 to 355.2152 deg, Dec +8.2029 to +19.5229 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 338.4279 to 355.2152 deg, Dec 8.2029 to 19.5229 deg
Loaded 6473 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): 4800 out of 5169 total matches.
Matched with Tycho-2 5169 out of 42031 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits:
Forced-photometry filter: calibrated wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits -> calib.txt_param_ref_wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits (aperture=5.1)
____ 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:
2.1 pix Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
2.4 pix Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
2.3 pix fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
2.3 pix fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
2.1 pix wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
2.4 pix wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
Limiting magnitude estimates:
15.2 mag. Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
15.1 mag. Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
13.4 mag. fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
13.4 mag. fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 12.9 (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.htIn9sbr14 (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_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits' -> 'wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
WCS-calibrated image found: wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
Checking if the catalog wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits
WCS catalog name: wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.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=9, blended=2139, bad_region=6661, passed=44698
Got 44698 stars (including 36229 good ones) from the SExtractor catalog wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat
util/solve_plate_with_UCAC5 got 44698 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4863 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 4850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 39755 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 39755 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4852 matched stars entering correct_measured_positions(), 39755 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4852 stars left (next iteration limit 5335)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits N_match=4852 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.346 sigma_q3_arcsec=0.423 sigma_q4_arcsec=0.372 n_q1=1495 n_q2=875 n_q3=1632 n_q4=850 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits -region wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.drB9s3y7eP (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits' -> 'wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
WCS_IMAGE_NAME=wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
WCS-calibrated image found: wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
Checking if the catalog wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits alredy exist and is non-empty...
Catalog wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat corresponding to the image wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits
WCS catalog name: wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.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=6, blended=1612, bad_region=6524, passed=42025
Got 42025 stars (including 34080 good ones) from the SExtractor catalog wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat
util/solve_plate_with_UCAC5 got 42025 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4866 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 4853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 36920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4866 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 36920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.21"
Accuracy estimation diagnostic: 4853 matched stars entering correct_measured_positions(), 36920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Excluding outliers - 4853 stars left (next iteration limit 5338)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits N_match=4853 sigma_overall_arcsec=0.229 sigma_q1_arcsec=0.249 sigma_q2_arcsec=0.224 sigma_q3_arcsec=0.228 sigma_q4_arcsec=0.203 n_q1=1509 n_q2=810 n_q3=1733 n_q4=801 worst_quadrant_to_overall_ratio=1.089
The image catalog is written to wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits -region wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8DfIXRY333 (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_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.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_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
Checking if the catalog wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
WCS catalog name: wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.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=2, blended=563, bad_region=2164, passed=13463
Got 13463 stars (including 11039 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat
util/solve_plate_with_UCAC5 got 13463 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4888 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 4875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 11829 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4888 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 11829 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 11829 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 4875 stars left (next iteration limit 5362)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits N_match=4875 sigma_overall_arcsec=0.475 sigma_q1_arcsec=0.453 sigma_q2_arcsec=0.542 sigma_q3_arcsec=0.432 sigma_q4_arcsec=0.528 n_q1=1454 n_q2=903 n_q3=1632 n_q4=886 worst_quadrant_to_overall_ratio=1.141
The image catalog is written to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits -region wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FUY5PxxD1W (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_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.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_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
WCS-calibrated image found: wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
Checking if the catalog wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat corresponding to the image wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
WCS catalog name: wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.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=1, blended=573, bad_region=2184, passed=13310
Got 13310 stars (including 10872 good ones) from the SExtractor catalog wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat
util/solve_plate_with_UCAC5 got 13310 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 4875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 11675 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 11675 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 11675 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 4875 stars left (next iteration limit 5362)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits N_match=4875 sigma_overall_arcsec=0.489 sigma_q1_arcsec=0.459 sigma_q2_arcsec=0.567 sigma_q3_arcsec=0.458 sigma_q4_arcsec=0.536 n_q1=1466 n_q2=902 n_q3=1617 n_q4=890 worst_quadrant_to_overall_ratio=1.160
The image catalog is written to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits -region wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.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_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-58-36_20.00sec_-0.00C_LIGHT_0012.fits
Saving fully-calibrated image wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.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_2026-07-29_CI_Peg-10-Q2b1x1_060059_TTUQ2b1x1_3286772_KkePwCyN/wcs_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013.fits
Preparing the HTML report for the field Peg-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:16:45.29 +10:37:35.1: 12.56 +/- 0.03 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:15:25.40 +10:56:59.4: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-06-12_05-06-41_20.00sec_5.00C_LIGHT_0287.fits at 23:02:38.09 +11:14:15.1: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:16:45.29 +10:37:35.1: 12.73 +/- 0.03 detection
Forced photometry on wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:02:38.09 +11:14:15.1: 15.72 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Forced photometry filter REJECTED candidate at 23:16:45.29 +10:37:35.1: ref_mag=12.64 +/- 0.02 new_mean_mag=12.4695 delta=0.17 (need > 0.90)
Forced photometry on wcs_Peg-10-Q2b1x1_2026-06-18_03-11-40_20.00sec_-0.00C_LIGHTs_0366.fits at 23:15:25.40 +10:56:59.4: 15.66 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out53294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53822.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 53294_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013
Preparing report for the candidate 53294_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013
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Considering the candidate 53822_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013
Preparing report for the candidate 53822_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013
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Considering the candidate 54417_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013
The candidate 54417_fd_Peg-10-Q2b1x1_2026-07-29_05-59-19_20.00sec_-0.00C_LIGHT_0013 did not pass the final checks