This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP
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 08 24.1013 2461276.6013 12.73 19:41:17.79 -16:37:51.8
23.20228 -18.33443 galactic Sgr Second-epoch detections are separated by 0.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.125 Liberatrix 0 -0 0 12.8 0 -0
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits at 19:41:17.79 -16:37:51.8: 15.15 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits at 19:41:17.79 -16:37:51.8: 15.21 +/- 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,2461276.6013,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260824.1013 12.73CV 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 08 24.1013 2461276.6013 11.64 19:27:02.62 -18:30:49.4
19.96614 -15.98435 galactic Sgr Second-epoch detections are separated by 3.1" and 8.6 pix
The object was found in VSX 1" AN Sgr
Type: M
# Max. Min./Amp. JD0 Period
8.860 V 14.500 V 2454645.00000 340.000000000000 M5e-M8
The object was not found in astcheck.
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits at 19:27:02.62 -18:30:49.4: 12.51 +/- 0.04 detection
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits at 19:27:02.62 -18:30:49.4: 12.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.03
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
AN Sgr,2461276.6013,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AN Sgr 20260824.1013 11.64CV 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: 2461176.84267280 16.05.2026 08:13:16.930 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
First image: 2461176.84267280 16.05.2026 08:13:16.930 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
Last image: 2461276.60172016 24.08.2026 02:26:18.622 /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.24
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 10827
Objects passed selection criteria: 10785
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 7666.75
Average stars matched: 7242.75 (94.4696 %)
Memory usage VmPeak: 236884 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 23 21:58:10 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: 2461176.84267280 16.05.2026 08:13:16.930 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
First image: 2461176.84267280 16.05.2026 08:13:16.930 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
Last image: 2461276.60172016 24.08.2026 02:26:18.622 /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 50
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 23 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 101137
Objects passed selection criteria: 100929
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 75501.5
Average stars matched: 71568.5 (94.7908 %)
Memory usage VmPeak: 566452 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 23 21:59:11 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
SExtractor catalog cache: saved Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.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/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.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: 2461276.60093926
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_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits exists and is non-empty
wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits exists and is non-empty
wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits exists and is non-empty
wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits (1st reference image)
verification OK: wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
Image size: 938.0'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:20.449 -17:59:40.25 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/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_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits (1st new image)
verification OK: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
Image size: 940.9'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:33:35.260 -17:59:23.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:20.449 -17:59:40.25
Second-epoch image center 19:33:35.260 -17:59:23.21
Angular distance between the image centers 0.0589 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits (2nd new image)
verification OK: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
Image size: 940.9'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:33:32.788 -17:58:48.82 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:20.449 -17:59:40.25
Second-epoch image center 19:33:32.788 -17:58:48.82
Angular distance between the image centers 0.0509 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 19:33:35.260 -17:59:23.21
Second-epoch second image center 19:33:32.788 -17:58:48.82
Angular distance between the image centers 0.01368 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/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits &> /tmp/tmp.WjZIZ7dYkP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits &> /tmp/tmp.OKJuXNcaCA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits &> /tmp/tmp.AOn8wlHMjR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits &> /tmp/tmp.9Pz04nmYct
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.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_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits and wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.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_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits and wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat
Found non-empty wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits and wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat
The reference image (wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits) and catalog (wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat) found
'wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat' -> 'wcsmag.cat'
Read 11241 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.8931 to 301.7273 deg, Dec -23.2641 to -12.5890 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 284.8931 to 301.7273 deg, Dec -23.2641 to -12.5890 deg
Loaded 13526 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): 8319 out of 8624 total matches.
Matched with Tycho-2 8624 out of 11241 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.533800
a=0.000000 b=1.000000 c=22.533800
From vast_summary.log: estimated ref. image limiting mag.: -8.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.29
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 11241 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.8931 to 301.7273 deg, Dec -23.2641 to -12.5890 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 284.8931 to 301.7273 deg, Dec -23.2641 to -12.5890 deg
Loaded 13526 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): 8319 out of 8624 total matches.
Matched with Tycho-2 8624 out of 11241 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
Forced-photometry filter: calibrated wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits -> calib.txt_param_ref_wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits (aperture=6.4)
Read 12331 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.9088 to 301.7295 deg, Dec -23.2926 to -12.6789 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 284.9088 to 301.7295 deg, Dec -23.2926 to -12.6789 deg
Loaded 13412 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): 8773 out of 9063 total matches.
Matched with Tycho-2 9063 out of 12331 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
Forced-photometry filter: calibrated wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits -> calib.txt_param_ref_wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
2.3 pix Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
2.7 pix fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
2.7 pix fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
Limiting magnitude estimates:
14.3 mag. Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
14.4 mag. Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
13.1 mag. fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
13.1 mag. fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 10.4 (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
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.WjZIZ7dYkP (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/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.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_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits' -> 'wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.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/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
Checking if the catalog wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
WCS catalog name: wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=821, bad_region=0, passed=11241
Got 11241 stars (including 10408 good ones) from the SExtractor catalog wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat
util/solve_plate_with_UCAC5 got 11241 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 4881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 11241 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
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 11241 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 11241 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 4880 stars left (next iteration limit 5369)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits N_match=4880 sigma_overall_arcsec=0.556 sigma_q1_arcsec=0.484 sigma_q2_arcsec=0.493 sigma_q3_arcsec=0.675 sigma_q4_arcsec=0.549 n_q1=1502 n_q2=954 n_q3=1485 n_q4=939 worst_quadrant_to_overall_ratio=1.213
The image catalog is written to wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits -region wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.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.OKJuXNcaCA (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/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.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_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits' -> 'wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.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/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
Checking if the catalog wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat corresponding to the image wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat corresponding to the image wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
WCS catalog name: wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=787, bad_region=0, passed=12331
Got 12331 stars (including 11533 good ones) from the SExtractor catalog wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat
util/solve_plate_with_UCAC5 got 12331 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 333 to 388 (Dec -23.3 to -12.7)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 4875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 12331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 333 to 388 (Dec -23.3 to -12.7)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 12331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 12331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 4874 stars left (next iteration limit 5361)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits N_match=4874 sigma_overall_arcsec=0.535 sigma_q1_arcsec=0.484 sigma_q2_arcsec=0.594 sigma_q3_arcsec=0.524 sigma_q4_arcsec=0.613 n_q1=1498 n_q2=885 n_q3=1546 n_q4=945 worst_quadrant_to_overall_ratio=1.145
The image catalog is written to wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits -region wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.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.AOn8wlHMjR (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_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.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_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
Checking if the catalog wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat corresponding to the image wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat corresponding to the image wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
WCS catalog name: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=528, bad_region=0, passed=3658
Got 3658 stars (including 3127 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat
util/solve_plate_with_UCAC5 got 3658 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 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 332 to 391 (Dec -23.5 to -12.2)
Done reading UCAC5 zone files...
Matched 3078 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3034 matched stars entering correct_measured_positions(), 3036 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3034 matched stars entering correct_measured_positions(), 3658 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 332 to 391 (Dec -23.5 to -12.2)
Done reading UCAC5 zone files...
Matched 3079 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3033 matched stars entering correct_measured_positions(), 3658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 3033 matched stars entering correct_measured_positions(), 3658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 3033 stars left (next iteration limit 3337)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3033 robust_rms=7.215 arcsec worst_quadrant_rms=20.025 arcsec
SIP_REFIT: SIP order 3 trial: matched=3033 robust_rms=0.408 arcsec worst_quadrant_rms=0.433 arcsec
SIP_REFIT: SIP order 5 trial: matched=3033 robust_rms=0.337 arcsec worst_quadrant_rms=0.386 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3033 robust_rms_before=0.883 arcsec robust_rms_before_corrected=0.396 arcsec robust_rms_after=0.337 arcsec worst_quadrant_rms_before=0.468 worst_quadrant_rms_after=0.386
verification OK: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
verification OK: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
Image size: 941.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:33:35.271 -17:59:24.08 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3658 stars ###
'wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/correct_sextractor_wcs_catalog_usingxy2sky1325116.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.883 -> 0.337 arcsec)
WCS_QUALITY_DIAG: file=fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits N_match=3033 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.388 sigma_q2_arcsec=0.360 sigma_q3_arcsec=0.331 sigma_q4_arcsec=0.334 n_q1=961 n_q2=578 n_q3=946 n_q4=548 worst_quadrant_to_overall_ratio=1.100
The image catalog is written to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits -region wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.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.9Pz04nmYct (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_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.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_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
Checking if the catalog wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat corresponding to the image wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat corresponding to the image wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
WCS catalog name: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=529, bad_region=0, passed=3640
Got 3640 stars (including 3107 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat
util/solve_plate_with_UCAC5 got 3640 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 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 332 to 391 (Dec -23.5 to -12.2)
Done reading UCAC5 zone files...
Matched 3063 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3023 matched stars entering correct_measured_positions(), 3024 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3023 matched stars entering correct_measured_positions(), 3640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.2)
Done reading UCAC5 zone files...
Matched 3065 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3022 matched stars entering correct_measured_positions(), 3640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 3022 matched stars entering correct_measured_positions(), 3640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 3022 stars left (next iteration limit 3325)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3022 robust_rms=7.230 arcsec worst_quadrant_rms=21.390 arcsec
SIP_REFIT: SIP order 3 trial: matched=3022 robust_rms=0.393 arcsec worst_quadrant_rms=0.417 arcsec
SIP_REFIT: SIP order 5 trial: matched=3022 robust_rms=0.322 arcsec worst_quadrant_rms=0.386 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3022 robust_rms_before=0.887 arcsec robust_rms_before_corrected=0.425 arcsec robust_rms_after=0.322 arcsec worst_quadrant_rms_before=0.486 worst_quadrant_rms_after=0.386
verification OK: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
verification OK: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
Image size: 941.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:33:32.804 -17:58:49.74 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3640 stars ###
'wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/correct_sextractor_wcs_catalog_usingxy2sky1325102.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.887 -> 0.322 arcsec)
WCS_QUALITY_DIAG: file=fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits N_match=3022 sigma_overall_arcsec=0.334 sigma_q1_arcsec=0.386 sigma_q2_arcsec=0.350 sigma_q3_arcsec=0.318 sigma_q4_arcsec=0.304 n_q1=961 n_q2=599 n_q3=925 n_q4=537 worst_quadrant_to_overall_ratio=1.155
The image catalog is written to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits -region wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits to local_wcs_cache/
'wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits'
Saving the final (post-refit) wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits to local_wcs_cache/
'wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits'
Saving the final (post-refit) wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits'
Saving the final (post-refit) wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits sigma_overall=0.556 worst_q_ratio=1.213
ref2=Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits sigma_overall=0.535 worst_q_ratio=1.145
new1=fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits sigma_overall=0.352 worst_q_ratio=1.100
new2=fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits sigma_overall=0.334 worst_q_ratio=1.155
reference average sigma_overall=0.5455 worst_q_ratio=1.179
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225_astrometric_residuals.png (4880 matched stars from wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040_astrometric_residuals.png (4874 matched stars from wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018_astrometric_residuals.png (3033 matched stars from wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019_astrometric_residuals.png (3022 matched stars from wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits'
Saving fully-calibrated image wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits'
Preparing the HTML report for the field Sgr-03-Q1b1x1 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 21634_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 21634_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:03:43.40 -15:56:36.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21663_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 21663_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:25:34.08 -20:06:54.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20047_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 20047_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:16:14.49 -16:58:17.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20136_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 20136_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:13:59.62 -17:25:54.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20034_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 20034_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:19:25.92 -19:01:25.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07778_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 07778_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:48:44.32 -15:58:23.6 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 Sgr-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
SExtractor catalog cache: saved Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
Creating symlink local_wcs_cache/wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits exists and is non-empty
wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits exists and is non-empty
wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits exists and is non-empty
wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits (1st reference image)
verification OK: wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
Image size: 938.0'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:20.449 -17:59:40.25 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/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_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits (1st new image)
verification OK: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
Image size: 941.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:33:35.271 -17:59:24.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:20.449 -17:59:40.25
Second-epoch image center 19:33:35.271 -17:59:24.08
Angular distance between the image centers 0.0589 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits (2nd new image)
verification OK: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
Image size: 941.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:33:32.804 -17:58:49.74 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:20.449 -17:59:40.25
Second-epoch image center 19:33:32.804 -17:58:49.74
Angular distance between the image centers 0.0509 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 19:33:35.271 -17:59:24.08
Second-epoch second image center 19:33:32.804 -17:58:49.74
Angular distance between the image centers 0.01366 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/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits &> /tmp/tmp.WmhR1h4oL4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits &> /tmp/tmp.5ZkZhv9f8o
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits &> /tmp/tmp.bPrkwLPSWz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits &> /tmp/tmp.0A5xJyusfv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.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_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits and wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.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_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits and wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat
Found non-empty wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits and wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat
The reference image (wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits) and catalog (wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat) found
'wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat' -> 'wcsmag.cat'
Read 114156 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.8761 to 301.8489 deg, Dec -23.2651 to -12.5890 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 284.8761 to 301.8489 deg, Dec -23.2651 to -12.5890 deg
Loaded 13576 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): 10044 out of 12010 total matches.
Matched with Tycho-2 12010 out of 114156 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.326250
a=0.000000 b=1.000000 c=22.326250
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.46
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 114156 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.8761 to 301.8489 deg, Dec -23.2651 to -12.5890 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 284.8761 to 301.8489 deg, Dec -23.2651 to -12.5890 deg
Loaded 13576 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): 10044 out of 12010 total matches.
Matched with Tycho-2 12010 out of 114156 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
Forced-photometry filter: calibrated wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits -> calib.txt_param_ref_wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits (aperture=4.6)
Read 114706 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.8931 to 301.8618 deg, Dec -23.2926 to -12.6438 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 284.8931 to 301.8618 deg, Dec -23.2926 to -12.6438 deg
Loaded 13517 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): 10140 out of 11918 total matches.
Matched with Tycho-2 11918 out of 114706 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
Forced-photometry filter: calibrated wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits -> calib.txt_param_ref_wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 44 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
2.2 pix Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
2.5 pix fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
2.5 pix fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
Limiting magnitude estimates:
14.5 mag. Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
14.5 mag. Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
13.3 mag. fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
13.3 mag. fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 12.7 (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.WmhR1h4oL4 (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/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.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_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits' -> 'wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.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/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
Checking if the catalog wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat corresponding to the image wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits
WCS catalog name: wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=9552, bad_region=2, passed=114126
Got 114126 stars (including 104423 good ones) from the SExtractor catalog wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat
util/solve_plate_with_UCAC5 got 114126 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 4889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 114126 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
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 114126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 114126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4889 stars left (next iteration limit 5377)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits N_match=4889 sigma_overall_arcsec=0.533 sigma_q1_arcsec=0.479 sigma_q2_arcsec=0.482 sigma_q3_arcsec=0.635 sigma_q4_arcsec=0.535 n_q1=1505 n_q2=1043 n_q3=1316 n_q4=1025 worst_quadrant_to_overall_ratio=1.193
The image catalog is written to wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits -region wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.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.5ZkZhv9f8o (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/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.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_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits' -> 'wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.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/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
WCS-calibrated image found: wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
Checking if the catalog wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat corresponding to the image wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat corresponding to the image wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits
WCS catalog name: wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=9136, bad_region=0, passed=114693
Got 114693 stars (including 105407 good ones) from the SExtractor catalog wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat
util/solve_plate_with_UCAC5 got 114693 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 4873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 114693 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 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 4927 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(), 114693 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 114693 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4874 stars left (next iteration limit 5360)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits N_match=4874 sigma_overall_arcsec=0.519 sigma_q1_arcsec=0.473 sigma_q2_arcsec=0.536 sigma_q3_arcsec=0.519 sigma_q4_arcsec=0.603 n_q1=1526 n_q2=895 n_q3=1476 n_q4=977 worst_quadrant_to_overall_ratio=1.163
The image catalog is written to wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits -region wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.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.bPrkwLPSWz (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_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.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_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
Checking if the catalog wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat corresponding to the image wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat corresponding to the image wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
WCS catalog name: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=1302, bad_region=0, passed=37622
Got 37622 stars (including 36271 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat
util/solve_plate_with_UCAC5 got 37622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 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 332 to 391 (Dec -23.5 to -12.1)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 4870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 37622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 332 to 391 (Dec -23.5 to -12.1)
Done reading UCAC5 zone files...
Matched 4931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 37622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 37622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4866 stars left (next iteration limit 5355)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4866 robust_rms=6.863 arcsec worst_quadrant_rms=22.372 arcsec
SIP_REFIT: SIP order 3 trial: matched=4866 robust_rms=0.436 arcsec worst_quadrant_rms=0.478 arcsec
SIP_REFIT: SIP order 5 trial: matched=4866 robust_rms=0.366 arcsec worst_quadrant_rms=0.438 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4866 robust_rms_before=0.367 arcsec robust_rms_before_corrected=0.396 arcsec robust_rms_after=0.366 arcsec worst_quadrant_rms_before=0.440 worst_quadrant_rms_after=0.438
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.440 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits N_match=4866 sigma_overall_arcsec=0.397 sigma_q1_arcsec=0.456 sigma_q2_arcsec=0.381 sigma_q3_arcsec=0.381 sigma_q4_arcsec=0.332 n_q1=1434 n_q2=846 n_q3=1640 n_q4=946 worst_quadrant_to_overall_ratio=1.147
The image catalog is written to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits -region wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.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.0A5xJyusfv (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_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.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_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
Checking if the catalog wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat corresponding to the image wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat corresponding to the image wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
WCS catalog name: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1499, bad_region=0, passed=37979
Got 37979 stars (including 36420 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat
util/solve_plate_with_UCAC5 got 37979 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 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 332 to 391 (Dec -23.5 to -12.1)
Done reading UCAC5 zone files...
Matched 4929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 4868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 37979 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 332 to 391 (Dec -23.5 to -12.1)
Done reading UCAC5 zone files...
Matched 4929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 37979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 37979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4865 stars left (next iteration limit 5352)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4865 robust_rms=6.920 arcsec worst_quadrant_rms=22.965 arcsec
SIP_REFIT: SIP order 3 trial: matched=4865 robust_rms=0.419 arcsec worst_quadrant_rms=0.461 arcsec
SIP_REFIT: SIP order 5 trial: matched=4865 robust_rms=0.347 arcsec worst_quadrant_rms=0.429 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4865 robust_rms_before=0.349 arcsec robust_rms_before_corrected=0.391 arcsec robust_rms_after=0.347 arcsec worst_quadrant_rms_before=0.420 worst_quadrant_rms_after=0.429
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.420 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits N_match=4865 sigma_overall_arcsec=0.381 sigma_q1_arcsec=0.471 sigma_q2_arcsec=0.377 sigma_q3_arcsec=0.359 sigma_q4_arcsec=0.314 n_q1=1447 n_q2=852 n_q3=1617 n_q4=949 worst_quadrant_to_overall_ratio=1.235
The image catalog is written to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits -region wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.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_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.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_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-25-11_20.00sec_-0.00C_LIGHTs_0018.fits
Saving fully-calibrated image wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.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_2026-08-23_CI_Sgr-03-Q1b1x1_215541_TTUQ1b1x1_1276233_3ROWmODP/wcs_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019.fits
Preparing the HTML report for the field Sgr-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits at 19:05:31.63 -12:42:40.7: 99.00 +/- 99.00 edge
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits at 19:01:52.03 -17:33:17.9: 11.79 +/- 0.02 detection
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits at 19:14:44.05 -18:05:00.7: 11.68 +/- 0.02 detection
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits at 19:06:12.15 -15:56:33.2: 12.91 +/- 0.06 detection
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits at 19:23:28.45 -12:44:50.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits at 19:23:28.45 -12:44:50.9: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 19:23:28.45 -12:44:50.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits at 19:11:03.29 -15:55:53.4: 12.03 +/- 0.03 detection
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits at 19:11:20.25 -12:43:24.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits at 19:11:20.25 -12:43:24.9: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 19:11:20.25 -12:43:24.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits at 19:05:31.63 -12:42:40.7: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 19:05:31.63 -12:42:40.7: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits at 19:06:12.15 -15:56:33.2: 12.78 +/- 0.06 detection
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits at 19:01:52.03 -17:33:17.9: 11.76 +/- 0.02 detection
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits at 19:14:44.05 -18:05:00.7: 11.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.04
Forced photometry reference-image weighted average: 11.77 +/- 0.02
Forced photometry filter REJECTED candidate at 19:06:12.15 -15:56:33.2: ref_mag=12.84 +/- 0.04 new_mean_mag=12.8753 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Forced photometry filter REJECTED candidate at 19:01:52.03 -17:33:17.9: ref_mag=11.77 +/- 0.02 new_mean_mag=12.2310 delta=-0.46 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:14:44.05 -18:05:00.7: ref_mag=11.77 +/- 0.01 new_mean_mag=12.2610 delta=-0.49 (need > 0.90)
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits at 19:11:03.29 -15:55:53.4: 12.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.02
Forced photometry filter REJECTED candidate at 19:11:03.29 -15:55:53.4: ref_mag=12.04 +/- 0.02 new_mean_mag=12.2590 delta=-0.22 (need > 0.90)
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits at 19:50:56.57 -22:37:05.6: 12.52 +/- 0.04 detection
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits at 19:41:17.79 -16:37:51.8: 15.15 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits at 19:50:56.57 -22:37:05.6: 12.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.03
Forced photometry filter REJECTED candidate at 19:50:56.57 -22:37:05.6: ref_mag=12.60 +/- 0.03 new_mean_mag=12.2860 delta=0.32 (need > 0.90)
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-05-16_03-13-16_20.00sec_-0.00C_LIGHT_0225.fits at 19:27:02.62 -18:30:49.4: 12.51 +/- 0.04 detection
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits at 19:41:17.79 -16:37:51.8: 15.21 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-03-Q1b1x1_2026-07-08_01-01-56_20.00sec_4.90C_LIGHT_0040.fits at 19:27:02.62 -18:30:49.4: 12.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.03
Forced photometry filter KEPT candidate at 19:27:02.62 -18:30:49.4: ref_mag=12.62 +/- 0.03 new_mean_mag=11.6404 delta=0.97 (need > 0.90)
Adding exclusion_list_local.txt__out139216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48622.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 138235_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138235_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
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Considering the candidate 138245_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138245_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
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Considering the candidate 138247_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138247_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
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Considering the candidate 138248_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138248_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:15:37.74 -17:28:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138253_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138253_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:29:33.28 -16:08:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138313_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138313_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
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Considering the candidate 138374_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138374_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:09:50.04 -20:59:50.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 138454_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138454_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
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Considering the candidate 138526_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138526_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:04:47.12 -22:16:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138571_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138571_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:25:10.32 -13:28:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138581_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138581_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:09:52.98 -20:59:57.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 138644_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138644_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
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Considering the candidate 138672_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138672_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:07:51.87 -13:14:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138772_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138772_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:06:05.88 -12:55:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138797_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138797_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
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Considering the candidate 138894_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138894_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:39:51.86 -15:11:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138917_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138917_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:17:30.70 -19:40:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138934_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138934_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:14:01.34 -14:01:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138937_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 138937_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:19:04.96 -19:34:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139032_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 139032_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:03:33.27 -15:16:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139042_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 139042_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:58:09.46 -14:57:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139043_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 139043_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
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Considering the candidate 139049_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 139049_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:36:26.15 -18:52:33.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 139148_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 139148_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:31:38.84 -15:30:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139216_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
Preparing report for the candidate 139216_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
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Considering the candidate 139290_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 139290_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:33:12.12 -14:48:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139394_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 139394_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:43:04.93 -21:00:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48622_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
Preparing report for the candidate 48622_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
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Considering the candidate 125469_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 125469_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:05:42.77 -18:41:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129180_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 129180_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:25:34.10 -20:06:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52293_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 52293_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:29:36.70 -18:16:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128593_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 128593_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:26:39.75 -17:06:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127126_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 127126_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:20:09.75 -20:41:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126429_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 126429_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:09:26.82 -16:32:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126332_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 126332_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:12:15.74 -18:29:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126088_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 126088_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:31:39.87 -17:57:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125838_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 125838_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:39:00.65 -16:51:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125807_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 125807_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:13:59.62 -17:25:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109935_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 109935_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:03:43.35 -15:56:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91456_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 91456_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:26:25.71 -14:06:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67607_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 67607_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:16:14.49 -16:58:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108737_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 108737_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:13:58.50 -15:53:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65839_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 65839_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks
**** FOUND 19:07:36.86 -17:01:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109419_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019
The candidate 109419_fd_Sgr-03-Q1b1x1_2026-08-23_21-26-18_20.00sec_-0.00C_LIGHTs_0019 did not pass the final checks