This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi
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 05.2129 2461226.7129 9.37 19:07:58.79 -09:12:12.9
26.56343 -7.83303 galactic Aql Second-epoch detections are separated by 0.9" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.18 Melpomene -1 -1 1 9.0 0 0
Forced photometry on wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits at 19:07:58.79 -09:12:12.9: 13.44 +/- 0.07 detection
Forced photometry on wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits at 19:07:58.79 -09:12:12.9: 13.57 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.05
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,2461226.7129,9.37,0.05,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 20260705.2129 9.37CV 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: 2461175.86862118 15.05.2026 08:50:38.870 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
First image: 2461175.86862118 15.05.2026 08:50:38.870 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
Last image: 2461226.71325995 05.07.2026 05:06:55.660 /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.12
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: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 12087
Objects passed selection criteria: 11972
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 6960.75
Average stars matched: 6722.25 (96.5736 %)
Memory usage VmPeak: 118840 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 3 15:05:03 CDT 2026
VaST build number 1.0rc89-123-g57107621
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jul 5 00:10:20 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 3
Ref. image: 2461175.86862118 15.05.2026 08:50:38.870 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
First image: 2461175.86862118 15.05.2026 08:50:38.870 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
Last image: 2461226.71325995 05.07.2026 05:06:55.660 /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.80
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: 25 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 150874
Objects passed selection criteria: 150438
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 3
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 3
Average stars detected per image: 118982
Average stars matched: 112580 (94.6191 %)
Memory usage VmPeak: 1925588 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Jul 3 15:05:03 CDT 2026
VaST build number 1.0rc89-123-g57107621
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jul 5 00:19:52 CDT 2026
Host name: tau
***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
SExtractor catalog cache: saved Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits.cat to cache
SExtractor catalog cache: saved Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.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/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_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: 2461226.71258559
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits exists and is non-empty
Saving wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits to local_wcs_cache/
'wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits' -> 'local_wcs_cache/wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits'
wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits exists and is non-empty
Saving wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits to local_wcs_cache/
'wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits' -> 'local_wcs_cache/wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits'
wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits exists and is non-empty
Saving wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits to local_wcs_cache/
'wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits' -> 'local_wcs_cache/wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits'
wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits exists and is non-empty
Saving wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits to local_wcs_cache/
'wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits' -> 'local_wcs_cache/wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits (1st reference image)
verification OK: wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
Image size: 937.3'x624.3' 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: 18:51:27.434 -09:59:38.01 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_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits (1st new image)
verification OK: wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits
Image size: 937.0'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:51:26.724 -10:00:10.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:27.434 -09:59:38.01
Second-epoch image center 18:51:26.724 -10:00:10.83
Angular distance between the image centers 0.0096 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits (2nd new image)
verification OK: wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
Image size: 937.0'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: 18:51:29.160 -09:59:22.18 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:51:27.434 -09:59:38.01
Second-epoch image center 18:51:29.160 -09:59:22.18
Angular distance between the image centers 0.0083 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 18:51:26.724 -10:00:10.83
Second-epoch second image center 18:51:29.160 -09:59:22.18
Angular distance between the image centers 0.01681 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/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits &> /tmp/tmp.05ij43lQYb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits &> /tmp/tmp.Bft5xXqReJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits &> /tmp/tmp.sK5geZ31zG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits &> /tmp/tmp.EtJ6ZixQGY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.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_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits and wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.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_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits and wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits.wcscat
Found non-empty wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits and wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits.wcscat
The reference image (wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits) and catalog (wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits.wcscat) found
'wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits.wcscat' -> 'wcsmag.cat'
Read 17086 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.8053 to 290.9470 deg, Dec -15.2603 to -4.6921 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 274.8053 to 290.9470 deg, Dec -15.2603 to -4.6921 deg
Loaded 13894 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): 9579 out of 10178 total matches.
Matched with Tycho-2 10178 out of 17086 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.701700
a=0.000000 b=1.000000 c=22.701700
From vast_summary.log: estimated ref. image limiting mag.: -8.12
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.58
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 17086 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.8053 to 290.9470 deg, Dec -15.2603 to -4.6921 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 274.8053 to 290.9470 deg, Dec -15.2603 to -4.6921 deg
Loaded 13894 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): 9579 out of 10178 total matches.
Matched with Tycho-2 10178 out of 17086 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits:
Forced-photometry filter: calibrated wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits -> calib.txt_param_ref_wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits (aperture=6.2)
Read 16932 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.8052 to 290.9459 deg, Dec -15.2634 to -4.6839 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 274.8052 to 290.9459 deg, Dec -15.2634 to -4.6839 deg
Loaded 13906 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): 9436 out of 10029 total matches.
Matched with Tycho-2 10029 out of 16932 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits:
Forced-photometry filter: calibrated wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits -> calib.txt_param_ref_wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
2.3 pix Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits
2.2 pix fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits
2.2 pix fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
2.3 pix wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
2.3 pix wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits
Limiting magnitude estimates:
14.6 mag. Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
14.6 mag. Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits
11.4 mag. fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits
11.4 mag. fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
All-image limiting magnitude estimate: 11.4 (SNR ) 9.4 (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.05ij43lQYb (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_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits' -> 'wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
WCS_IMAGE_NAME=wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
WCS-calibrated image found: wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
Checking if the catalog wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits.wcscat corresponding to the image wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits alredy exist and is non-empty...
Catalog wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits.wcscat corresponding to the image wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits
WCS catalog name: wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.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=1405, bad_region=3848, passed=17086
Got 17086 stars (including 12043 good ones) from the SExtractor catalog wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits.wcscat
util/solve_plate_with_UCAC5 got 17086 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 13277 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 13278 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 13277 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits N_match=938 sigma_overall_arcsec=0.536 sigma_q1_arcsec=0.519 sigma_q2_arcsec=0.537 sigma_q3_arcsec=0.561 sigma_q4_arcsec=0.495 n_q1=311 n_q2=192 n_q3=224 n_q4=211 worst_quadrant_to_overall_ratio=1.046
The image catalog is written to wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits -region wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.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.Bft5xXqReJ (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_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits' -> 'wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits
WCS_IMAGE_NAME=wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits
WCS-calibrated image found: wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits
Checking if the catalog wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits.wcscat corresponding to the image wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits alredy exist and is non-empty...
Catalog wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits.wcscat corresponding to the image wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits
WCS catalog name: wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.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=1412, bad_region=3812, passed=16932
Got 16932 stars (including 11917 good ones) from the SExtractor catalog wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits.wcscat
util/solve_plate_with_UCAC5 got 16932 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 13175 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 13174 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 13174 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits N_match=936 sigma_overall_arcsec=0.527 sigma_q1_arcsec=0.504 sigma_q2_arcsec=0.557 sigma_q3_arcsec=0.581 sigma_q4_arcsec=0.491 n_q1=306 n_q2=197 n_q3=220 n_q4=213 worst_quadrant_to_overall_ratio=1.103
The image catalog is written to wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits -region wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.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.sK5geZ31zG (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_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_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_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits
WCS-calibrated image found: wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits
Checking if the catalog wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits.wcscat corresponding to the image wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits.wcscat corresponding to the image wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits
WCS catalog name: wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_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=50, bad_region=182, passed=1000
Got 1000 stars (including 772 good ones) from the SExtractor catalog wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits.wcscat
util/solve_plate_with_UCAC5 got 1000 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 725 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 718 matched stars entering correct_measured_positions(), 694 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 718 matched stars entering correct_measured_positions(), 799 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 726 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 718 matched stars entering correct_measured_positions(), 800 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 718 matched stars entering correct_measured_positions(), 800 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 718 stars left (next iteration limit 789)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits N_match=718 sigma_overall_arcsec=0.567 sigma_q1_arcsec=0.560 sigma_q2_arcsec=0.710 sigma_q3_arcsec=0.569 sigma_q4_arcsec=0.546 n_q1=179 n_q2=82 n_q3=265 n_q4=192 worst_quadrant_to_overall_ratio=1.251
The image catalog is written to wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits -region wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_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.EtJ6ZixQGY (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_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_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_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
WCS-calibrated image found: wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
Checking if the catalog wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits.wcscat corresponding to the image wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits.wcscat corresponding to the image wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
WCS catalog name: wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_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=58, bad_region=209, passed=1054
Got 1054 stars (including 796 good ones) from the SExtractor catalog wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits.wcscat
util/solve_plate_with_UCAC5 got 1054 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 747 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 742 matched stars entering correct_measured_positions(), 720 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 742 matched stars entering correct_measured_positions(), 841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 747 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 742 matched stars entering correct_measured_positions(), 839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 742 matched stars entering correct_measured_positions(), 839 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 742 stars left (next iteration limit 816)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits N_match=742 sigma_overall_arcsec=0.602 sigma_q1_arcsec=0.676 sigma_q2_arcsec=0.771 sigma_q3_arcsec=0.549 sigma_q4_arcsec=0.596 n_q1=201 n_q2=84 n_q3=260 n_q4=197 worst_quadrant_to_overall_ratio=1.280
The image catalog is written to wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits -region wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_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=Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits sigma_overall=0.536 worst_q_ratio=1.046
ref2=Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits sigma_overall=0.527 worst_q_ratio=1.103
new1=fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits sigma_overall=0.567 worst_q_ratio=1.251
new2=fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits sigma_overall=0.602 worst_q_ratio=1.280
reference average sigma_overall=0.5315 worst_q_ratio=1.0745
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129_astrometric_residuals.png (938 matched stars from wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.47 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130_astrometric_residuals.png (936 matched stars from wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012_astrometric_residuals.png (718 matched stars from wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.53 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013_astrometric_residuals.png (742 matched stars from wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.52 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-05-57_20.00sec_4.90C_LIGHT_0012.fits'
Saving fully-calibrated image wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-05_CI_Sct-01-Q2b1x1_000728_TTUQ2b1x1_3349213_NsAIpJHi/wcs_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013.fits'
Preparing the HTML report for the field Sct-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Sct-01-Q2b1x1_2026-05-15_03-50-38_20.00sec_-0.00C_LIGHT_0129.fits at 19:07:58.79 -09:12:12.9: 13.44 +/- 0.07 detection
Forced photometry on wcs_Sct-01-Q2b1x1_2026-05-15_03-51-21_20.00sec_-0.00C_LIGHT_0130.fits at 19:07:58.79 -09:12:12.9: 13.57 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.05
Forced photometry filter KEPT candidate at 19:07:58.79 -09:12:12.9: ref_mag=13.49 +/- 0.05 new_mean_mag=9.3636 delta=4.13 (need > 0.90)
Adding exclusion_list_local.txt__out20952.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 85s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20952_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013
Preparing report for the candidate 20952_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013
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Considering the candidate 20953_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013
The candidate 20953_fd_Sct-01-Q2b1x1_2026-07-05_00-06-55_20.00sec_5.00C_LIGHT_0013 did not pass the final checks