This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 01.3465 2461284.8465 12.53 02:10:41.34 +28:44:03.0
143.21887 -30.99657 galactic Tri Second-epoch detections are separated by 0.9" 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.375 Ursula -0 -1 1 12.6 0 0
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:10:41.34 +28:44:03.0: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 02:10:41.34 +28:44:03.0: 15.85 +/- 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!
TCP 2026 09 01.3465* 02 10 41.34 +28 44 03.0 12.5 U Tri 9 0
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,2461284.8465,12.53,0.05,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 20260901.3465 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 01.3465 2461284.8465 13.26 01:52:19.24 +25:34:49.0
139.79676 -35.28970 galactic Ari Second-epoch detections are separated by 1.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1620 Geographos -2 -1 3 13.8 0 0
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:52:19.24 +25:34:49.0: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 01:52:19.24 +25:34:49.0: 15.81 +/- 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!
TCP 2026 09 01.3465* 01 52 19.24 +25 34 49.0 13.3 U Ari 9 0
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,2461284.8465,13.26,0.05,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 20260901.3465 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 01.3465 2461284.8465 13.78 01:52:38.06 +33:18:09.2
137.37454 -27.84711 galactic Tri Second-epoch detections are separated by 2.1" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.726 Joella -0 0 0 13.5 0 0
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:52:38.06 +33:18:09.2: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 01:52:38.06 +33:18:09.2: 15.71 +/- 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!
TCP 2026 09 01.3465* 01 52 38.06 +33 18 09.2 13.8 U Tri 9 0
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,2461284.8465,13.78,0.05,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 20260901.3465 13.78CV 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: 2461049.65440406 09.01.2026 03:42:10.511 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
First image: 2461049.65440406 09.01.2026 03:42:10.511 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Last image: 2461284.84679214 01.09.2026 08:19:12.841 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 3 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): 9561
Objects passed selection criteria: 9547
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: 7109.75
Average stars matched: 7047.5 (99.1244 %)
Memory usage VmPeak: 236468 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 1 03:24:05 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: 2461049.65440406 09.01.2026 03:42:10.511 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
First image: 2461049.65440406 09.01.2026 03:42:10.511 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Last image: 2461284.84679214 01.09.2026 08:19:12.841 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 11 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): 56907
Objects passed selection criteria: 56785
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 45052.2
Average stars matched: 44345.2 (98.4307 %)
Memory usage VmPeak: 282540 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Sep 1 03:24:50 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/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
SExtractor catalog cache: saved Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.cat to cache
SExtractor catalog cache: saved Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.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/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.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: 2461284.84619220
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits exists and is non-empty
wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits exists and is non-empty
wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits exists and is non-empty
wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits (1st reference image)
verification OK: wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Image size: 941.6'x627.0' 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: 02:00:00.767 +29:59:43.74 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits (1st new image)
verification OK: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
Image size: 941.2'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: 02:00:00.367 +30:01:02.71 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:00:00.767 +29:59:43.74
Second-epoch image center 02:00:00.367 +30:01:02.71
Angular distance between the image centers 0.0220 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits (2nd new image)
verification OK: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
Image size: 941.2'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: 01:59:57.537 +30:01:36.64 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:00:00.767 +29:59:43.74
Second-epoch image center 01:59:57.537 +30:01:36.64
Angular distance between the image centers 0.0335 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 02:00:00.367 +30:01:02.71
Second-epoch second image center 01:59:57.537 +30:01:36.64
Angular distance between the image centers 0.01389 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/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits &> /tmp/tmp.AP6hPD4OFJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits &> /tmp/tmp.Wme60fOUPt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits &> /tmp/tmp.jT5KMnK6HG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits &> /tmp/tmp.vQGfiNdyZh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
Calibrating the magnitude scale
Found non-empty wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
Found non-empty wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
The reference image (wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits) and catalog (wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat) found
'wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat' -> 'wcsmag.cat'
Read 12225 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.6031 to 39.6626 deg, Dec +24.4125 to +35.2960 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 20.6031 to 39.6626 deg, Dec 24.4125 to 35.2960 deg
Loaded 8372 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): 6352 out of 6781 total matches.
Matched with Tycho-2 6781 out of 12225 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.928900
a=0.000000 b=1.000000 c=22.928900
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 12225 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.6031 to 39.6626 deg, Dec +24.4125 to +35.2960 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 20.6031 to 39.6626 deg, Dec 24.4125 to 35.2960 deg
Loaded 8372 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): 6352 out of 6781 total matches.
Matched with Tycho-2 6781 out of 12225 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Forced-photometry filter: calibrated wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits -> calib.txt_param_ref_wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits (aperture=6.0)
Read 9704 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.4683 to 39.4466 deg, Dec +24.4124 to +35.2593 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 20.4683 to 39.4466 deg, Dec 24.4124 to 35.2593 deg
Loaded 8305 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): 6209 out of 6464 total matches.
Matched with Tycho-2 6464 out of 9704 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
Forced-photometry filter: calibrated wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits -> calib.txt_param_ref_wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
2.4 pix Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
2.3 pix fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
2.3 pix fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
Limiting magnitude estimates:
15.4 mag. Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
15.0 mag. Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
13.7 mag. fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
13.7 mag. fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 10.8 (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.AP6hPD4OFJ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits' -> 'wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS-calibrated image found: wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Checking if the catalog wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS catalog name: wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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=932, bad_region=0, passed=12225
Got 12225 stars (including 11278 good ones) from the SExtractor catalog wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
util/solve_plate_with_UCAC5 got 12225 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4850 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 4835 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 12225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4850 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 12225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 12225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4835 stars left (next iteration limit 5318)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits N_match=4835 sigma_overall_arcsec=0.283 sigma_q1_arcsec=0.361 sigma_q2_arcsec=0.262 sigma_q3_arcsec=0.267 sigma_q4_arcsec=0.239 n_q1=1307 n_q2=1363 n_q3=1097 n_q4=1068 worst_quadrant_to_overall_ratio=1.277
The image catalog is written to wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits -region wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Wme60fOUPt (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/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.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_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits' -> 'wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.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/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
WCS-calibrated image found: wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
Checking if the catalog wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat corresponding to the image wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat corresponding to the image wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
WCS catalog name: wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.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=660, bad_region=0, passed=9704
Got 9704 stars (including 9036 good ones) from the SExtractor catalog wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat
util/solve_plate_with_UCAC5 got 9704 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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4843 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 4830 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 9704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4842 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 9704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 9704 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4829 stars left (next iteration limit 5313)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits N_match=4829 sigma_overall_arcsec=0.479 sigma_q1_arcsec=0.387 sigma_q2_arcsec=0.501 sigma_q3_arcsec=0.509 sigma_q4_arcsec=0.476 n_q1=1048 n_q2=1135 n_q3=1321 n_q4=1325 worst_quadrant_to_overall_ratio=1.063
The image catalog is written to wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits -region wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.jT5KMnK6HG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
Checking if the catalog wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
WCS catalog name: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.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=437, bad_region=1, passed=3339
Got 3339 stars (including 2894 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat
util/solve_plate_with_UCAC5 got 3339 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (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 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 2800 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2795 matched stars entering correct_measured_positions(), 2795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2795 matched stars entering correct_measured_positions(), 3339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 2800 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2795 matched stars entering correct_measured_positions(), 3339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 2795 matched stars entering correct_measured_positions(), 3339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 2795 stars left (next iteration limit 3074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2795 robust_rms=10.348 arcsec worst_quadrant_rms=11.690 arcsec
SIP_REFIT: SIP order 3 trial: matched=2795 robust_rms=0.379 arcsec worst_quadrant_rms=0.401 arcsec
SIP_REFIT: SIP order 5 trial: matched=2795 robust_rms=0.292 arcsec worst_quadrant_rms=0.298 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2795 robust_rms_before=1.046 arcsec robust_rms_before_corrected=0.329 arcsec robust_rms_after=0.292 arcsec worst_quadrant_rms_before=0.348 worst_quadrant_rms_after=0.298
verification OK: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
verification OK: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
Image size: 941.3'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: 02:00:00.401 +30:01:01.95 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3339 stars ###
'wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/correct_sextractor_wcs_catalog_usingxy2sky884736.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.046 -> 0.292 arcsec)
WCS_QUALITY_DIAG: file=fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits N_match=2795 sigma_overall_arcsec=0.315 sigma_q1_arcsec=0.338 sigma_q2_arcsec=0.321 sigma_q3_arcsec=0.315 sigma_q4_arcsec=0.298 n_q1=602 n_q2=633 n_q3=822 n_q4=738 worst_quadrant_to_overall_ratio=1.072
The image catalog is written to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits -region wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.vQGfiNdyZh (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
Checking if the catalog wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
WCS catalog name: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.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=443, bad_region=0, passed=3350
Got 3350 stars (including 2904 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat
util/solve_plate_with_UCAC5 got 3350 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (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 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 2813 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2808 matched stars entering correct_measured_positions(), 2808 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2808 matched stars entering correct_measured_positions(), 3350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 2813 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2808 matched stars entering correct_measured_positions(), 3350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 2808 matched stars entering correct_measured_positions(), 3350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 2808 stars left (next iteration limit 3088)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2808 robust_rms=10.697 arcsec worst_quadrant_rms=12.013 arcsec
SIP_REFIT: SIP order 3 trial: matched=2808 robust_rms=0.384 arcsec worst_quadrant_rms=0.386 arcsec
SIP_REFIT: SIP order 5 trial: matched=2808 robust_rms=0.276 arcsec worst_quadrant_rms=0.284 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2808 robust_rms_before=1.030 arcsec robust_rms_before_corrected=0.313 arcsec robust_rms_after=0.276 arcsec worst_quadrant_rms_before=0.327 worst_quadrant_rms_after=0.284
verification OK: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
verification OK: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
Image size: 941.3'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: 01:59:57.572 +30:01:35.86 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3350 stars ###
'wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/correct_sextractor_wcs_catalog_usingxy2sky884735.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.030 -> 0.276 arcsec)
WCS_QUALITY_DIAG: file=fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits N_match=2808 sigma_overall_arcsec=0.298 sigma_q1_arcsec=0.320 sigma_q2_arcsec=0.317 sigma_q3_arcsec=0.290 sigma_q4_arcsec=0.285 n_q1=605 n_q2=642 n_q3=828 n_q4=733 worst_quadrant_to_overall_ratio=1.073
The image catalog is written to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits -region wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits to local_wcs_cache/
'wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits' -> 'local_wcs_cache/wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits'
Saving the final (post-refit) wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits to local_wcs_cache/
'wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits' -> 'local_wcs_cache/wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits'
Saving the final (post-refit) wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits to local_wcs_cache/
'wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits' -> 'local_wcs_cache/wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits'
Saving the final (post-refit) wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits to local_wcs_cache/
'wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits' -> 'local_wcs_cache/wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits sigma_overall=0.283 worst_q_ratio=1.277
ref2=Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits sigma_overall=0.479 worst_q_ratio=1.063
new1=fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits sigma_overall=0.315 worst_q_ratio=1.072
new2=fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits sigma_overall=0.298 worst_q_ratio=1.073
reference average sigma_overall=0.381 worst_q_ratio=1.17
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113_astrometric_residuals.png (4835 matched stars from wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365_astrometric_residuals.png (4829 matched stars from wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352_astrometric_residuals.png (2795 matched stars from wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353_astrometric_residuals.png (2808 matched stars from wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits'
Saving fully-calibrated image wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits'
Preparing the HTML report for the field Tri-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11861_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 11861_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 02:16:07.11 +25:03:24.0 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 Tri-01-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/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
SExtractor catalog cache: saved Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.cat to cache
SExtractor catalog cache: saved Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Creating symlink local_wcs_cache/wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
Creating symlink local_wcs_cache/wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
Creating symlink local_wcs_cache/wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.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_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits exists and is non-empty
wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits exists and is non-empty
wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits exists and is non-empty
wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits (1st reference image)
verification OK: wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Image size: 941.6'x627.0' 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: 02:00:00.767 +29:59:43.74 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits (1st new image)
verification OK: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
Image size: 941.3'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: 02:00:00.401 +30:01:01.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:00:00.767 +29:59:43.74
Second-epoch image center 02:00:00.401 +30:01:01.95
Angular distance between the image centers 0.0218 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits (2nd new image)
verification OK: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
Image size: 941.3'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: 01:59:57.572 +30:01:35.86 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:00:00.767 +29:59:43.74
Second-epoch image center 01:59:57.572 +30:01:35.86
Angular distance between the image centers 0.0332 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 02:00:00.401 +30:01:01.95
Second-epoch second image center 01:59:57.572 +30:01:35.86
Angular distance between the image centers 0.01389 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/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits &> /tmp/tmp.UOehP9Elm2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits &> /tmp/tmp.duDvkIpfdW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits &> /tmp/tmp.NL6aap3R76
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits &> /tmp/tmp.CqfT24tJC7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
Calibrating the magnitude scale
Found non-empty wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
Found non-empty wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
The reference image (wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits) and catalog (wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat) found
'wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat' -> 'wcsmag.cat'
Read 73246 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.5706 to 39.6918 deg, Dec +24.3217 to +35.3065 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 20.5706 to 39.6918 deg, Dec 24.3217 to 35.3065 deg
Loaded 8459 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): 5808 out of 6890 total matches.
Matched with Tycho-2 6890 out of 73246 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.815100
a=0.000000 b=1.000000 c=22.815100
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.58
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 73246 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.5706 to 39.6918 deg, Dec +24.3217 to +35.3065 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 20.5706 to 39.6918 deg, Dec 24.3217 to 35.3065 deg
Loaded 8459 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): 5808 out of 6890 total matches.
Matched with Tycho-2 6890 out of 73246 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Forced-photometry filter: calibrated wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits -> calib.txt_param_ref_wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits (aperture=4.7)
Read 58792 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.4130 to 39.4510 deg, Dec +24.4125 to +35.2639 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 20.4130 to 39.4510 deg, Dec 24.4125 to 35.2639 deg
Loaded 8329 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): 6052 out of 6815 total matches.
Matched with Tycho-2 6815 out of 58792 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
Forced-photometry filter: calibrated wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits -> calib.txt_param_ref_wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 26 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
2.1 pix Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
2.2 pix fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
2.2 pix fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
Limiting magnitude estimates:
15.6 mag. Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
15.2 mag. Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
13.9 mag. fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
13.9 mag. fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.3 (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.UOehP9Elm2 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits' -> 'wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS-calibrated image found: wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Checking if the catalog wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS catalog name: wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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=17, blended=4778, bad_region=6, passed=73229
Got 73229 stars (including 68317 good ones) from the SExtractor catalog wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
util/solve_plate_with_UCAC5 got 73229 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 4847 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 4835 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 73229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 4847 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 73229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 73229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4835 stars left (next iteration limit 5318)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits N_match=4835 sigma_overall_arcsec=0.279 sigma_q1_arcsec=0.355 sigma_q2_arcsec=0.265 sigma_q3_arcsec=0.259 sigma_q4_arcsec=0.235 n_q1=1268 n_q2=1372 n_q3=1109 n_q4=1086 worst_quadrant_to_overall_ratio=1.270
The image catalog is written to wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits -region wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.duDvkIpfdW (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/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.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_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits' -> 'wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.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/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
WCS-calibrated image found: wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
Checking if the catalog wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat corresponding to the image wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat corresponding to the image wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits
WCS catalog name: wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.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=32, blended=3229, bad_region=1, passed=58760
Got 58760 stars (including 55458 good ones) from the SExtractor catalog wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat
util/solve_plate_with_UCAC5 got 58760 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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4839 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 4825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 58760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4838 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4826 matched stars entering correct_measured_positions(), 58760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4826 matched stars entering correct_measured_positions(), 58760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4826 stars left (next iteration limit 5307)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.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_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits N_match=4826 sigma_overall_arcsec=0.456 sigma_q1_arcsec=0.363 sigma_q2_arcsec=0.480 sigma_q3_arcsec=0.487 sigma_q4_arcsec=0.456 n_q1=1054 n_q2=1140 n_q3=1270 n_q4=1362 worst_quadrant_to_overall_ratio=1.067
The image catalog is written to wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits -region wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.NL6aap3R76 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
Checking if the catalog wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
WCS catalog name: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.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=5, blended=796, bad_region=1, passed=24699
Got 24699 stars (including 23860 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat
util/solve_plate_with_UCAC5 got 24699 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 4847 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 4831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 24699 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 4847 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 24699 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 24699 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4831 stars left (next iteration limit 5314)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.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=4831 robust_rms=9.873 arcsec worst_quadrant_rms=11.194 arcsec
SIP_REFIT: SIP order 3 trial: matched=4831 robust_rms=0.400 arcsec worst_quadrant_rms=0.416 arcsec
SIP_REFIT: SIP order 5 trial: matched=4831 robust_rms=0.312 arcsec worst_quadrant_rms=0.324 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4831 robust_rms_before=0.314 arcsec robust_rms_before_corrected=0.331 arcsec robust_rms_after=0.312 arcsec worst_quadrant_rms_before=0.326 worst_quadrant_rms_after=0.324
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.326 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits N_match=4831 sigma_overall_arcsec=0.346 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.376 sigma_q3_arcsec=0.342 sigma_q4_arcsec=0.324 n_q1=1063 n_q2=1090 n_q3=1395 n_q4=1283 worst_quadrant_to_overall_ratio=1.086
The image catalog is written to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits -region wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.CqfT24tJC7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
Checking if the catalog wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
WCS catalog name: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.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=3, blended=789, bad_region=0, passed=24687
Got 24687 stars (including 23855 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat
util/solve_plate_with_UCAC5 got 24687 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 4831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 24687 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 24687 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 24687 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4831 stars left (next iteration limit 5314)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.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=4831 robust_rms=9.933 arcsec worst_quadrant_rms=11.396 arcsec
SIP_REFIT: SIP order 3 trial: matched=4831 robust_rms=0.404 arcsec worst_quadrant_rms=0.420 arcsec
SIP_REFIT: SIP order 5 trial: matched=4831 robust_rms=0.302 arcsec worst_quadrant_rms=0.308 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4831 robust_rms_before=0.303 arcsec robust_rms_before_corrected=0.320 arcsec robust_rms_after=0.302 arcsec worst_quadrant_rms_before=0.311 worst_quadrant_rms_after=0.308
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.311 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits N_match=4831 sigma_overall_arcsec=0.334 sigma_q1_arcsec=0.339 sigma_q2_arcsec=0.360 sigma_q3_arcsec=0.317 sigma_q4_arcsec=0.330 n_q1=1070 n_q2=1089 n_q3=1388 n_q4=1284 worst_quadrant_to_overall_ratio=1.078
The image catalog is written to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits -region wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-18-21_20.00sec_0.00C_LIGHTs_0352.fits
Saving fully-calibrated image wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-01_CI_Tri-01-Q1b1x1_032136_TTUQ1b1x1_869650_pZrqxGTv/wcs_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353.fits
Preparing the HTML report for the field Tri-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:53:02.97 +31:31:24.4: 12.16 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:36:02.77 +31:48:06.7: 12.09 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:37:33.71 +30:33:08.4: 12.46 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:10:41.34 +28:44:03.0: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:52:27.23 +27:14:49.4: 11.48 +/- 0.00 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:56:14.56 +27:29:14.3: 12.33 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:39:05.23 +28:21:29.0: 12.67 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:08:13.90 +24:48:00.5: 12.07 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:04:52.38 +31:08:57.9: 12.78 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:03:37.09 +27:29:57.3: 12.86 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 01:39:05.23 +28:21:29.0: 12.57 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 01:37:33.71 +30:33:08.4: 12.38 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 01:36:02.77 +31:48:06.7: 11.75 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 01:56:14.56 +27:29:14.3: 12.39 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 01:53:02.97 +31:31:24.4: 12.21 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 02:08:13.90 +24:48:00.5: 12.12 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 01:52:27.23 +27:14:49.4: 11.40 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 02:10:41.34 +28:44:03.0: 15.85 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter REJECTED candidate at 01:36:02.77 +31:48:06.7: ref_mag=11.93 +/- 0.01 new_mean_mag=12.2976 delta=-0.37 (need > 0.90)
Forced photometry reference-image weighted average: 11.45 +/- 0.00
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Forced photometry filter REJECTED candidate at 01:53:02.97 +31:31:24.4: ref_mag=12.17 +/- 0.01 new_mean_mag=12.5333 delta=-0.36 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:56:14.56 +27:29:14.3: ref_mag=12.35 +/- 0.01 new_mean_mag=12.5843 delta=-0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:39:05.23 +28:21:29.0: ref_mag=12.63 +/- 0.01 new_mean_mag=12.9559 delta=-0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:37:33.71 +30:33:08.4: ref_mag=12.43 +/- 0.01 new_mean_mag=12.4481 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:52:27.23 +27:14:49.4: ref_mag=11.45 +/- 0.00 new_mean_mag=11.7504 delta=-0.30 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:08:13.90 +24:48:00.5: ref_mag=12.09 +/- 0.01 new_mean_mag=12.0702 delta=0.02 (need > 0.90)
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 02:04:52.38 +31:08:57.9: 12.77 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 02:03:37.09 +27:29:57.3: 12.84 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Forced photometry filter REJECTED candidate at 02:04:52.38 +31:08:57.9: ref_mag=12.77 +/- 0.02 new_mean_mag=12.8985 delta=-0.13 (need > 0.90)
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry filter REJECTED candidate at 02:03:37.09 +27:29:57.3: ref_mag=12.85 +/- 0.02 new_mean_mag=12.8789 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:36:51.95 +29:25:14.3: 12.97 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:53:09.30 +28:50:27.5: 12.95 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:35:24.20 +34:21:07.9: 12.83 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:58:56.09 +34:21:17.2: 13.25 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:52:19.24 +25:34:49.0: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:16:39.72 +29:47:02.8: 12.67 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:58:48.20 +32:51:28.5: 13.42 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:52:38.06 +33:18:09.2: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:23:59.07 +33:30:44.5: 12.60 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 02:16:39.72 +29:47:02.8: 12.86 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 01:52:19.24 +25:34:49.0: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 01:53:09.30 +28:50:27.5: 12.76 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 01:58:56.09 +34:21:17.2: 13.19 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 01:58:48.20 +32:51:28.5: 13.35 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 01:36:51.95 +29:25:14.3: 12.71 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 02:35:24.20 +34:21:07.9: 13.20 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry reference-image weighted average: 13.23 +/- 0.03
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Forced photometry filter REJECTED candidate at 01:58:48.20 +32:51:28.5: ref_mag=13.39 +/- 0.03 new_mean_mag=13.4823 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry filter REJECTED candidate at 02:16:39.72 +29:47:02.8: ref_mag=12.73 +/- 0.01 new_mean_mag=13.0530 delta=-0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:53:09.30 +28:50:27.5: ref_mag=12.87 +/- 0.02 new_mean_mag=13.0990 delta=-0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:58:56.09 +34:21:17.2: ref_mag=13.23 +/- 0.03 new_mean_mag=13.1095 delta=0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:35:24.20 +34:21:07.9: ref_mag=12.92 +/- 0.02 new_mean_mag=12.9662 delta=-0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:36:51.95 +29:25:14.3: ref_mag=12.85 +/- 0.02 new_mean_mag=13.1053 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 01:52:38.06 +33:18:09.2: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 02:23:59.07 +33:30:44.5: 12.70 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Forced photometry filter REJECTED candidate at 02:23:59.07 +33:30:44.5: ref_mag=12.63 +/- 0.02 new_mean_mag=12.7233 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Tri-01-Q1b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:11:12.16 +30:07:31.2: 13.14 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q1b1x1_2026-07-14_05-20-24_20.00sec_5.00C_LIGHT_0365.fits at 02:11:12.16 +30:07:31.2: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter REJECTED candidate at 02:11:12.16 +30:07:31.2: ref_mag=13.16 +/- 0.02 new_mean_mag=13.1482 delta=0.01 (need > 0.90)
Adding exclusion_list_local.txt__out85793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85994.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 3s
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Considering the candidate 85572_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85572_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85575_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85575_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85577_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85577_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85578_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85578_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85579_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85579_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 01:43:40.82 +28:03:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85701_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85701_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 01:53:01.07 +29:36:56.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 85715_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85715_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85750_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85750_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85791_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85791_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85793_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
Preparing report for the candidate 85793_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
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Considering the candidate 85840_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85840_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85843_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85843_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85845_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85845_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 02:17:06.20 +34:11:29.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 85880_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85880_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85885_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85885_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85892_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85892_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85905_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85905_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85910_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85910_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85950_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
Preparing report for the candidate 85950_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
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Considering the candidate 85959_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85959_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 01:53:14.75 +29:35:41.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 85967_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85967_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 85994_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
Preparing report for the candidate 85994_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
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Considering the candidate 85061_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 85061_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 84944_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 84944_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 57866_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 57866_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 01:31:48.29 +26:40:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51017_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353
The candidate 51017_fd_Tri-01-Q1b1x1_2026-09-01_03-19-12_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks