This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc
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 10 07.3060 2461320.8060 10.69 06:49:38.58 +48:17:01.2
167.87670 19.61695 galactic Aur Second-epoch detections are separated by 0.3" and 6.9 pix
The object was found in VSX 1" CD Aur
Type: M
# Max. Min./Amp. JD0 Period
12.600 pg < 16.500 pg 2427800.00000 334.500000000000 M6/7
The object was not found in astcheck.
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:49:38.58 +48:17:01.2: 11.52 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:49:38.58 +48:17:01.2: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CD Aur,2461320.8060,10.69,0.05,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
CD Aur 20261007.3060 10.69CV 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 10 07.3060 2461320.8060 12.95 06:43:36.88 +42:38:29.8
173.04882 16.65121 galactic Aur Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.61 Danae -0 -0 0 13.2 0 0
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:43:36.88 +42:38:29.8: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:43:36.88 +42:38:29.8: 15.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461320.8060,12.95,0.05,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 20261007.3060 12.95CV 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: 2461058.75756060 18.01.2026 06:10:43.236 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
First image: 2461058.75756060 18.01.2026 06:10:43.236 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Last image: 2461320.80640230 07.10.2026 07:21:03.159 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.25
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: 19 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): 14988
Objects passed selection criteria: 14980
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 14588.8
Average stars matched: 14171.2 (97.1382 %)
Memory usage VmPeak: 240628 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 7 08:42:37 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.75756060 18.01.2026 06:10:43.236 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
First image: 2461058.75756060 18.01.2026 06:10:43.236 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Last image: 2461320.80640230 07.10.2026 07:21:03.159 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 86
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -6.95
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: 199 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): 95615
Objects passed selection criteria: 95429
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 88801.5
Average stars matched: 85523.2 (96.3083 %)
Memory usage VmPeak: 559144 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 7 08:47:41 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/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
SExtractor catalog cache: saved Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat to cache
SExtractor catalog cache: saved Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.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/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_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
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: 2461320.80561944
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits exists and is non-empty
wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits exists and is non-empty
wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits exists and is non-empty
wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits (1st reference image)
verification OK: wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Image size: 941.8'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:11:58.091 +45:59:39.02 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_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits (1st new image)
verification OK: wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
Image size: 942.1'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: 07:11:48.303 +46:01:25.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:11:58.091 +45:59:39.02
Second-epoch image center 07:11:48.303 +46:01:25.10
Angular distance between the image centers 0.0409 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits (2nd new image)
verification OK: wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
Image size: 942.1'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: 07:11:51.289 +46:01:55.81 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:11:58.091 +45:59:39.02
Second-epoch image center 07:11:51.289 +46:01:55.81
Angular distance between the image centers 0.0428 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 07:11:48.303 +46:01:25.10
Second-epoch second image center 07:11:51.289 +46:01:55.81
Angular distance between the image centers 0.01214 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/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits &> /tmp/tmp.egxnSjugrg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits &> /tmp/tmp.EpE1DveI6m
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits &> /tmp/tmp.lp5WogjyA0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits &> /tmp/tmp.ffY7ecVYcq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.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_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits and wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.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_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits and wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat
Found non-empty wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits and wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat
The reference image (wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits) and catalog (wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat) found
'wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat' -> 'wcsmag.cat'
Read 16801 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.2052 to 119.8634 deg, Dec +39.8309 to +51.4020 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 95.2052 to 119.8634 deg, Dec 39.8309 to 51.4020 deg
Loaded 8911 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): 5895 out of 6499 total matches.
Matched with Tycho-2 6499 out of 16801 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.913800
a=0.000000 b=1.000000 c=22.913800
From vast_summary.log: estimated ref. image limiting mag.: -7.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.66
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.66
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 16801 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.2052 to 119.8634 deg, Dec +39.8309 to +51.4020 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 95.2052 to 119.8634 deg, Dec 39.8309 to 51.4020 deg
Loaded 8911 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): 5895 out of 6499 total matches.
Matched with Tycho-2 6499 out of 16801 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Forced-photometry filter: calibrated wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits -> calib.txt_param_ref_wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits (aperture=6.2)
Read 15355 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.9342 to 120.4944 deg, Dec +39.9653 to +51.3502 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 95.9342 to 120.4944 deg, Dec 39.9653 to 51.3502 deg
Loaded 8532 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): 5920 out of 6428 total matches.
Matched with Tycho-2 6428 out of 15355 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
Forced-photometry filter: calibrated wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits -> calib.txt_param_ref_wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 12 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
2.2 pix Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
2.6 pix fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
2.6 pix fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
Limiting magnitude estimates:
15.7 mag. Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
15.6 mag. Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
15.2 mag. fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
15.2 mag. fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.1 (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.egxnSjugrg (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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits' -> 'wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.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/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
WCS_IMAGE_NAME=wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
WCS-calibrated image found: wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Checking if the catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits alredy exist and is non-empty...
Catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
WCS catalog name: wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.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=1405, bad_region=0, passed=16801
Got 16801 stars (including 15373 good ones) from the SExtractor catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat
util/solve_plate_with_UCAC5 got 16801 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4856 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 4838 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 16801 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 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4857 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 16801 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 16801 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4838 stars left (next iteration limit 5320)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits N_match=4838 sigma_overall_arcsec=0.339 sigma_q1_arcsec=0.410 sigma_q2_arcsec=0.316 sigma_q3_arcsec=0.328 sigma_q4_arcsec=0.277 n_q1=1362 n_q2=1097 n_q3=1306 n_q4=1073 worst_quadrant_to_overall_ratio=1.210
The image catalog is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits -region wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.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.EpE1DveI6m (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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits' -> 'wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.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/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
WCS-calibrated image found: wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
Checking if the catalog wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits.wcscat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits.wcscat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
WCS catalog name: wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.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=1203, bad_region=0, passed=15355
Got 15355 stars (including 14132 good ones) from the SExtractor catalog wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits.wcscat
util/solve_plate_with_UCAC5 got 15355 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4849 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 15355 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4849 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 15355 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 15355 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4830 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_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits N_match=4830 sigma_overall_arcsec=0.365 sigma_q1_arcsec=0.500 sigma_q2_arcsec=0.370 sigma_q3_arcsec=0.332 sigma_q4_arcsec=0.312 n_q1=972 n_q2=1329 n_q3=1079 n_q4=1450 worst_quadrant_to_overall_ratio=1.367
The image catalog is written to wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits -region wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.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.lp5WogjyA0 (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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
Checking if the catalog wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits.wcscat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits.wcscat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_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_Lyn-03-Q1b1x1_2026-10-07_02-19-55_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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
WCS catalog name: wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_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=715, bad_region=0, passed=13284
Got 13284 stars (including 12555 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits.wcscat
util/solve_plate_with_UCAC5 got 13284 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 4842 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 4823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 13284 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
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: 4825 matched stars entering correct_measured_positions(), 13284 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 13284 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4824 stars left (next iteration limit 5305)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4824 robust_rms=11.997 arcsec worst_region_rms=29.481 arcsec outer_annulus_rms=29.481 arcsec
SIP_REFIT: SIP order 3 trial: matched=4824 robust_rms=0.553 arcsec worst_region_rms=0.777 arcsec outer_annulus_rms=0.777 arcsec
SIP_REFIT: SIP order 5 trial: matched=4824 robust_rms=0.378 arcsec worst_region_rms=0.491 arcsec outer_annulus_rms=0.491 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4824 robust_rms_before=0.964 arcsec robust_rms_before_corrected=0.348 arcsec robust_rms_after=0.378 arcsec worst_region_rms_before=0.534 worst_region_rms_after=0.491 outer_annulus_rms_before=0.996 outer_annulus_rms_after=0.491
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.534 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits worst_region_rms_kept=0.534 arcsec robust_rms_kept=0.348 arcsec matched=4824
WCS_QUALITY_DIAG: file=fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits N_match=4824 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.339 sigma_q2_arcsec=0.384 sigma_q3_arcsec=0.321 sigma_q4_arcsec=0.381 n_q1=1480 n_q2=972 n_q3=1400 n_q4=972 worst_quadrant_to_overall_ratio=1.097
The image catalog is written to wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits -region wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_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.ffY7ecVYcq (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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
Checking if the catalog wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_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_Lyn-03-Q1b1x1_2026-10-07_02-21-03_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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
WCS catalog name: wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_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=700, bad_region=0, passed=13266
Got 13266 stars (including 12547 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat
util/solve_plate_with_UCAC5 got 13266 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 649 to 708 (Dec 39.9 to 51.4)
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: 4824 matched stars entering correct_measured_positions(), 4824 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 13266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 649 to 708 (Dec 39.9 to 51.4)
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: 4824 matched stars entering correct_measured_positions(), 13266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 13266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4824 stars left (next iteration limit 5306)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4824 robust_rms=11.928 arcsec worst_region_rms=30.203 arcsec outer_annulus_rms=30.203 arcsec
SIP_REFIT: SIP order 3 trial: matched=4824 robust_rms=0.450 arcsec worst_region_rms=0.834 arcsec outer_annulus_rms=0.834 arcsec
SIP_REFIT: SIP order 5 trial: matched=4824 robust_rms=0.355 arcsec worst_region_rms=0.490 arcsec outer_annulus_rms=0.490 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4824 robust_rms_before=0.935 arcsec robust_rms_before_corrected=0.325 arcsec robust_rms_after=0.355 arcsec worst_region_rms_before=0.527 worst_region_rms_after=0.490 outer_annulus_rms_before=0.932 outer_annulus_rms_after=0.490
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.527 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits worst_region_rms_kept=0.527 arcsec robust_rms_kept=0.325 arcsec matched=4824
WCS_QUALITY_DIAG: file=fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits N_match=4824 sigma_overall_arcsec=0.322 sigma_q1_arcsec=0.314 sigma_q2_arcsec=0.375 sigma_q3_arcsec=0.278 sigma_q4_arcsec=0.343 n_q1=1485 n_q2=974 n_q3=1391 n_q4=974 worst_quadrant_to_overall_ratio=1.163
The image catalog is written to wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits -region wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_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_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits to local_wcs_cache/
'wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits' -> 'local_wcs_cache/wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits'
Saving the final (post-refit) wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits to local_wcs_cache/
'wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits' -> 'local_wcs_cache/wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits'
Saving the final (post-refit) wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits to local_wcs_cache/
'wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits' -> 'local_wcs_cache/wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits'
Saving the final (post-refit) wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits to local_wcs_cache/
'wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits' -> 'local_wcs_cache/wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits sigma_overall=0.339 worst_q_ratio=1.210
ref2=Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits sigma_overall=0.365 worst_q_ratio=1.367
new1=fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits sigma_overall=0.350 worst_q_ratio=1.097
new2=fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits sigma_overall=0.322 worst_q_ratio=1.163
reference average sigma_overall=0.352 worst_q_ratio=1.2885
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258_astrometric_residuals.png (4838 matched stars from wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233_astrometric_residuals.png (4830 matched stars from wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352_astrometric_residuals.png (4824 matched stars from wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353_astrometric_residuals.png (4824 matched stars from wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits'
Saving fully-calibrated image wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits'
Preparing the HTML report for the field Lyn-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:12:53.38 +47:23:13.7: 12.52 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:30:42.41 +45:26:58.0: 11.67 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:08:47.81 +44:25:31.0: 12.36 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:05:56.49 +47:42:06.9: 12.48 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:05:07.74 +45:09:28.7: 12.47 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:49:38.58 +48:17:01.2: 11.52 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 07:08:47.81 +44:25:31.0: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter REJECTED candidate at 07:08:47.81 +44:25:31.0: ref_mag=12.38 +/- 0.01 new_mean_mag=12.3842 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 07:05:56.49 +47:42:06.9: 12.48 +/- 0.01 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:30:42.41 +45:26:58.0: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry filter REJECTED candidate at 07:05:56.49 +47:42:06.9: ref_mag=12.48 +/- 0.01 new_mean_mag=12.4365 delta=0.04 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:30:42.41 +45:26:58.0: ref_mag=11.64 +/- 0.01 new_mean_mag=12.0429 delta=-0.40 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 07:12:53.38 +47:23:13.7: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Forced photometry filter REJECTED candidate at 07:12:53.38 +47:23:13.7: ref_mag=12.51 +/- 0.01 new_mean_mag=12.4974 delta=0.01 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:49:38.58 +48:17:01.2: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Forced photometry filter KEPT candidate at 06:49:38.58 +48:17:01.2: ref_mag=11.64 +/- 0.01 new_mean_mag=10.6904 delta=0.95 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 07:05:07.74 +45:09:28.7: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry filter REJECTED candidate at 07:05:07.74 +45:09:28.7: ref_mag=12.46 +/- 0.01 new_mean_mag=12.3516 delta=0.11 (need > 0.90)
Adding exclusion_list_local.txt__out12738.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21522_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 21522_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21586_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 21586_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:01:33.32 +43:54:17.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21589_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 21589_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21599_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 21599_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21604_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 21604_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21612_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 21612_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12738_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
Preparing report for the candidate 12738_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10249_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 10249_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:10:45.16 +47:02:50.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21131_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 21131_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:26:02.66 +50:29:26.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10828_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 10828_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:31:42.46 +47:33:22.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03201_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 03201_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:20:33.60 +42:35:03.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11378_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 11378_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:57:09.09 +47:35:21.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 16s
Prepared the HTML report for the field Lyn-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:49:38.58 +48:17:01.2
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/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
SExtractor catalog cache: saved Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.cat to cache
SExtractor catalog cache: saved Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_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_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Creating symlink local_wcs_cache/wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
Checking 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_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits exists and is non-empty
wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits exists and is non-empty
wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits exists and is non-empty
wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits (1st reference image)
verification OK: wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Image size: 941.8'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:11:58.091 +45:59:39.02 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_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits (1st new image)
verification OK: wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
Image size: 942.1'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: 07:11:48.303 +46:01:25.10 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:11:58.091 +45:59:39.02
Second-epoch image center 07:11:48.303 +46:01:25.10
Angular distance between the image centers 0.0409 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits (2nd new image)
verification OK: wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
Image size: 942.1'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: 07:11:51.289 +46:01:55.81 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:11:58.091 +45:59:39.02
Second-epoch image center 07:11:51.289 +46:01:55.81
Angular distance between the image centers 0.0428 deg.
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# 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 07:11:48.303 +46:01:25.10
Second-epoch second image center 07:11:51.289 +46:01:55.81
Angular distance between the image centers 0.01214 deg.
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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/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits &> /tmp/tmp.nG4JwUDy5W
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits &> /tmp/tmp.KTr9X5XTpT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits &> /tmp/tmp.nCXXB9l48r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits &> /tmp/tmp.VkCbgJp3Ok
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.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_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits and wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.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_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits and wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat
Found non-empty wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits and wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat
The reference image (wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits) and catalog (wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat) found
'wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat' -> 'wcsmag.cat'
Read 108521 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.2052 to 119.8836 deg, Dec +39.7733 to +51.4069 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 95.2052 to 119.8836 deg, Dec 39.7733 to 51.4069 deg
Loaded 8995 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): 5098 out of 6518 total matches.
Matched with Tycho-2 6518 out of 108521 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.781950
a=0.000000 b=1.000000 c=22.781950
From vast_summary.log: estimated ref. image limiting mag.: -6.95
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.83
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.83
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 108521 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.2052 to 119.8836 deg, Dec +39.7733 to +51.4069 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 95.2052 to 119.8836 deg, Dec 39.7733 to 51.4069 deg
Loaded 8995 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): 5098 out of 6518 total matches.
Matched with Tycho-2 6518 out of 108521 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Forced-photometry filter: calibrated wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits -> calib.txt_param_ref_wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits (aperture=4.7)
Read 101005 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.9046 to 120.6246 deg, Dec +39.9534 to +51.3536 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 95.9046 to 120.6246 deg, Dec 39.9534 to 51.3536 deg
Loaded 8602 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): 5203 out of 6473 total matches.
Matched with Tycho-2 6473 out of 101005 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
Forced-photometry filter: calibrated wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits -> calib.txt_param_ref_wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 82 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
2.0 pix Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
2.5 pix fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
2.5 pix fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
Limiting magnitude estimates:
15.8 mag. Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
15.7 mag. Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
15.3 mag. fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
15.3 mag. fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.4 (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.nG4JwUDy5W (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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits' -> 'wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.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/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
WCS_IMAGE_NAME=wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
WCS-calibrated image found: wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
Checking if the catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits alredy exist and is non-empty...
Catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits
WCS catalog name: wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.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=33, blended=9545, bad_region=1, passed=108488
Got 108488 stars (including 98736 good ones) from the SExtractor catalog wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat
util/solve_plate_with_UCAC5 got 108488 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4848 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(), 4836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 108488 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 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4848 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(), 108488 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 108488 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.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_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits N_match=4835 sigma_overall_arcsec=0.325 sigma_q1_arcsec=0.396 sigma_q2_arcsec=0.305 sigma_q3_arcsec=0.309 sigma_q4_arcsec=0.274 n_q1=1340 n_q2=1118 n_q3=1281 n_q4=1096 worst_quadrant_to_overall_ratio=1.218
The image catalog is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits -region wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.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.KTr9X5XTpT (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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits' -> 'wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.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/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
WCS-calibrated image found: wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
Checking if the catalog wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits.wcscat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits.wcscat corresponding to the image wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits
WCS catalog name: wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.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=38, blended=7786, bad_region=3, passed=100967
Got 100967 stars (including 92994 good ones) from the SExtractor catalog wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits.wcscat
util/solve_plate_with_UCAC5 got 100967 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4840 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4828 matched stars entering correct_measured_positions(), 4828 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4828 matched stars entering correct_measured_positions(), 100967 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 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 4840 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(), 100967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 100967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4829 stars left (next iteration limit 5310)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.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_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits N_match=4829 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.476 sigma_q2_arcsec=0.365 sigma_q3_arcsec=0.321 sigma_q4_arcsec=0.292 n_q1=987 n_q2=1307 n_q3=1103 n_q4=1432 worst_quadrant_to_overall_ratio=1.353
The image catalog is written to wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits -region wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.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.nCXXB9l48r (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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
Checking if the catalog wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits.wcscat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits.wcscat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_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_Lyn-03-Q1b1x1_2026-10-07_02-19-55_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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
WCS catalog name: wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_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=4339, bad_region=46, passed=74148
Got 74148 stars (including 69639 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits.wcscat
util/solve_plate_with_UCAC5 got 74148 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 4833 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 4817 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 74148 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 4833 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 74148 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 74148 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4817 stars left (next iteration limit 5298)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_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=4817 robust_rms=11.959 arcsec worst_region_rms=30.360 arcsec outer_annulus_rms=30.360 arcsec
SIP_REFIT: SIP order 3 trial: matched=4817 robust_rms=0.562 arcsec worst_region_rms=0.777 arcsec outer_annulus_rms=0.777 arcsec
SIP_REFIT: SIP order 5 trial: matched=4817 robust_rms=0.375 arcsec worst_region_rms=0.491 arcsec outer_annulus_rms=0.491 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4817 robust_rms_before=0.953 arcsec robust_rms_before_corrected=0.343 arcsec robust_rms_after=0.375 arcsec worst_region_rms_before=0.511 worst_region_rms_after=0.491 outer_annulus_rms_before=0.990 outer_annulus_rms_after=0.491
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.511 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits worst_region_rms_kept=0.511 arcsec robust_rms_kept=0.343 arcsec matched=4817
WCS_QUALITY_DIAG: file=fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits N_match=4817 sigma_overall_arcsec=0.349 sigma_q1_arcsec=0.332 sigma_q2_arcsec=0.382 sigma_q3_arcsec=0.311 sigma_q4_arcsec=0.373 n_q1=1476 n_q2=967 n_q3=1378 n_q4=996 worst_quadrant_to_overall_ratio=1.094
The image catalog is written to wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits -region wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_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.VkCbgJp3Ok (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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
Checking if the catalog wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat corresponding to the image wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_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_Lyn-03-Q1b1x1_2026-10-07_02-21-03_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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
WCS catalog name: wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_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=10, blended=4373, bad_region=47, passed=74126
Got 74126 stars (including 69597 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat
util/solve_plate_with_UCAC5 got 74126 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 4831 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 4813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 74126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 4830 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 74126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 74126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4813 stars left (next iteration limit 5294)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_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=4813 robust_rms=11.926 arcsec worst_region_rms=30.657 arcsec outer_annulus_rms=30.657 arcsec
SIP_REFIT: SIP order 3 trial: matched=4813 robust_rms=0.450 arcsec worst_region_rms=0.842 arcsec outer_annulus_rms=0.842 arcsec
SIP_REFIT: SIP order 5 trial: matched=4813 robust_rms=0.355 arcsec worst_region_rms=0.498 arcsec outer_annulus_rms=0.498 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4813 robust_rms_before=0.928 arcsec robust_rms_before_corrected=0.320 arcsec robust_rms_after=0.355 arcsec worst_region_rms_before=0.502 worst_region_rms_after=0.498 outer_annulus_rms_before=0.924 outer_annulus_rms_after=0.498
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.502 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits worst_region_rms_kept=0.502 arcsec robust_rms_kept=0.320 arcsec matched=4813
WCS_QUALITY_DIAG: file=fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits N_match=4813 sigma_overall_arcsec=0.325 sigma_q1_arcsec=0.318 sigma_q2_arcsec=0.370 sigma_q3_arcsec=0.282 sigma_q4_arcsec=0.356 n_q1=1480 n_q2=959 n_q3=1370 n_q4=1004 worst_quadrant_to_overall_ratio=1.140
The image catalog is written to wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits -region wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_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_Lyn-03-Q1b1x1_2026-10-07_02-19-55_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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-19-55_20.00sec_-0.00C_LIGHTs_0352.fits
Saving fully-calibrated image wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_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_2026-10-07_CI_Lyn-03-Q1b1x1_025222_TTUQ1b1x1_2037808_igtlJqkc/wcs_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353.fits
Preparing the HTML report for the field Lyn-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:56:28.42 +44:09:26.7: 15.11 +/- 0.13 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:43:46.27 +48:40:53.7: 14.11 +/- 0.06 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:03:46.32 +50:23:43.9: 14.74 +/- 0.09 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:29:56.15 +46:53:08.0: 14.79 +/- 0.14 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:17:30.69 +41:17:28.0: 14.24 +/- 0.06 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:56:30.90 +45:39:16.2: 14.66 +/- 0.08 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:27:05.92 +47:39:37.5: 14.80 +/- 0.12 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:52:02.29 +48:22:54.0: 15.13 +/- 0.14 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:37:46.31 +50:27:53.2: 14.77 +/- 0.12 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:57:52.90 +50:32:57.0: 14.36 +/- 0.07 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:52:02.29 +48:22:54.0: 14.84 +/- 0.12 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:56:30.90 +45:39:16.2: 14.57 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.09
Forced photometry filter REJECTED candidate at 06:52:02.29 +48:22:54.0: ref_mag=14.97 +/- 0.09 new_mean_mag=14.9002 delta=0.07 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 07:43:46.27 +48:40:53.7: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.62 +/- 0.06
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:27:05.92 +47:39:37.5: 14.32 +/- 0.09 detection
Forced photometry filter REJECTED candidate at 06:56:30.90 +45:39:16.2: ref_mag=14.62 +/- 0.06 new_mean_mag=14.5527 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 14.14 +/- 0.04
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 07:03:46.32 +50:23:43.9: 14.65 +/- 0.10 detection
Forced photometry filter REJECTED candidate at 07:43:46.27 +48:40:53.7: ref_mag=14.14 +/- 0.04 new_mean_mag=14.1898 delta=-0.05 (need > 0.90)
Forced photometry reference-image weighted average: 14.50 +/- 0.07
Forced photometry filter REJECTED candidate at 06:27:05.92 +47:39:37.5: ref_mag=14.50 +/- 0.07 new_mean_mag=14.5914 delta=-0.09 (need > 0.90)
Forced photometry reference-image weighted average: 14.70 +/- 0.07
Forced photometry filter REJECTED candidate at 07:03:46.32 +50:23:43.9: ref_mag=14.70 +/- 0.07 new_mean_mag=14.6795 delta=0.02 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:57:52.90 +50:32:57.0: 14.47 +/- 0.08 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:37:46.31 +50:27:53.2: 14.79 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.40 +/- 0.05
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:56:28.42 +44:09:26.7: 15.23 +/- 0.16 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:29:56.15 +46:53:08.0: 14.93 +/- 0.17 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 07:17:30.69 +41:17:28.0: 14.13 +/- 0.06 detection
Forced photometry filter REJECTED candidate at 06:57:52.90 +50:32:57.0: ref_mag=14.40 +/- 0.05 new_mean_mag=14.4259 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 14.19 +/- 0.04
Forced photometry reference-image weighted average: 14.78 +/- 0.09
Forced photometry reference-image weighted average: 14.84 +/- 0.11
Forced photometry filter REJECTED candidate at 07:17:30.69 +41:17:28.0: ref_mag=14.19 +/- 0.04 new_mean_mag=14.2984 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:37:46.31 +50:27:53.2: ref_mag=14.78 +/- 0.09 new_mean_mag=14.6783 delta=0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:29:56.15 +46:53:08.0: ref_mag=14.84 +/- 0.11 new_mean_mag=14.9205 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 15.16 +/- 0.10
Forced photometry filter REJECTED candidate at 06:56:28.42 +44:09:26.7: ref_mag=15.16 +/- 0.10 new_mean_mag=15.0208 delta=0.14 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:42:46.41 +43:12:42.8: 13.98 +/- 0.05 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:31:57.41 +47:49:45.0: 14.44 +/- 0.08 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:44:53.03 +44:18:54.8: 14.52 +/- 0.08 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:50:00.54 +43:31:59.0: 13.94 +/- 0.05 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:43:36.88 +42:38:29.8: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:31:57.41 +47:49:45.0: 14.49 +/- 0.10 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:42:46.41 +43:12:42.8: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.06
Forced photometry filter REJECTED candidate at 06:31:57.41 +47:49:45.0: ref_mag=14.46 +/- 0.06 new_mean_mag=14.4120 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 13.89 +/- 0.03
Forced photometry filter REJECTED candidate at 06:42:46.41 +43:12:42.8: ref_mag=13.89 +/- 0.03 new_mean_mag=14.2098 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:50:00.54 +43:31:59.0: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Forced photometry filter REJECTED candidate at 06:50:00.54 +43:31:59.0: ref_mag=13.85 +/- 0.03 new_mean_mag=13.9775 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:44:53.03 +44:18:54.8: 14.52 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.06
Forced photometry filter REJECTED candidate at 06:44:53.03 +44:18:54.8: ref_mag=14.52 +/- 0.06 new_mean_mag=14.4886 delta=0.03 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:43:36.88 +42:38:29.8: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:54:30.92 +44:03:48.3: 13.35 +/- 0.03 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:43:01.48 +44:29:17.1: 13.26 +/- 0.03 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:43:01.48 +44:29:17.1: 13.26 +/- 0.04 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:54:30.92 +44:03:48.3: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Forced photometry filter REJECTED candidate at 06:43:01.48 +44:29:17.1: ref_mag=13.26 +/- 0.03 new_mean_mag=13.3591 delta=-0.10 (need > 0.90)
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter REJECTED candidate at 06:54:30.92 +44:03:48.3: ref_mag=13.31 +/- 0.02 new_mean_mag=13.3367 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:40:41.88 +44:54:25.7: 13.88 +/- 0.05 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:40:41.88 +44:54:25.7: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.03
Forced photometry filter REJECTED candidate at 06:40:41.88 +44:54:25.7: ref_mag=13.85 +/- 0.03 new_mean_mag=13.8012 delta=0.05 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:43:03.44 +44:29:13.8: 13.62 +/- 0.05 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:43:03.44 +44:29:13.8: 13.60 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.04
Forced photometry filter REJECTED candidate at 06:43:03.44 +44:29:13.8: ref_mag=13.61 +/- 0.04 new_mean_mag=13.7843 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:31:17.59 +42:34:16.1: 14.17 +/- 0.07 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:31:17.59 +42:34:16.1: 14.18 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.05
Forced photometry filter REJECTED candidate at 06:31:17.59 +42:34:16.1: ref_mag=14.17 +/- 0.05 new_mean_mag=14.0463 delta=0.12 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:49:55.79 +44:30:20.1: 14.34 +/- 0.07 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:49:55.79 +44:30:20.1: 14.37 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.05
Forced photometry filter REJECTED candidate at 06:49:55.79 +44:30:20.1: ref_mag=14.35 +/- 0.05 new_mean_mag=14.2413 delta=0.11 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:37:20.31 +47:33:52.1: 15.11 +/- 0.15 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:36:12.81 +50:23:02.2: 14.88 +/- 0.13 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:34:22.98 +41:29:33.2: 14.95 +/- 0.17 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:37:20.31 +47:33:52.1: 15.20 +/- 0.19 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:29:54.74 +48:17:07.0: 15.02 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.12
Forced photometry filter REJECTED candidate at 06:37:20.31 +47:33:52.1: ref_mag=15.15 +/- 0.12 new_mean_mag=14.7880 delta=0.36 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:47:11.42 +45:01:52.8: 15.26 +/- 0.17 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:36:12.81 +50:23:02.2: 15.05 +/- 0.19 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:38:31.72 +45:00:49.6: 14.93 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.11
Forced photometry filter REJECTED candidate at 06:36:12.81 +50:23:02.2: ref_mag=14.94 +/- 0.11 new_mean_mag=14.7617 delta=0.18 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:37:57.19 +43:32:46.3: 15.03 +/- 0.15 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:34:22.98 +41:29:33.2: 14.90 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.12
Forced photometry filter REJECTED candidate at 06:34:22.98 +41:29:33.2: ref_mag=14.92 +/- 0.12 new_mean_mag=14.6146 delta=0.31 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:47:11.42 +45:01:52.8: 15.11 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.12
Forced photometry filter REJECTED candidate at 06:47:11.42 +45:01:52.8: ref_mag=15.19 +/- 0.12 new_mean_mag=14.8259 delta=0.36 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:38:31.72 +45:00:49.6: 15.06 +/- 0.16 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:37:57.19 +43:32:46.3: 14.89 +/- 0.15 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:29:54.74 +48:17:07.0: 14.71 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.10
Forced photometry reference-image weighted average: 14.96 +/- 0.11
Forced photometry filter REJECTED candidate at 06:38:31.72 +45:00:49.6: ref_mag=14.98 +/- 0.10 new_mean_mag=14.7258 delta=0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:37:57.19 +43:32:46.3: ref_mag=14.96 +/- 0.11 new_mean_mag=14.8803 delta=0.08 (need > 0.90)
Forced photometry reference-image weighted average: 14.84 +/- 0.10
Forced photometry filter REJECTED candidate at 06:29:54.74 +48:17:07.0: ref_mag=14.84 +/- 0.10 new_mean_mag=14.8354 delta=0.00 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:32:02.06 +43:40:57.9: 14.97 +/- 0.14 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:32:02.06 +43:40:57.9: 14.75 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.10
Forced photometry filter REJECTED candidate at 06:32:02.06 +43:40:57.9: ref_mag=14.86 +/- 0.10 new_mean_mag=14.8921 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 07:00:35.33 +46:35:59.9: 15.18 +/- 0.14 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-01-18_00-10-43_20.00sec_-15.00C_LIGHT_0258.fits at 06:46:21.44 +45:49:29.4: 15.18 +/- 0.15 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 07:00:35.33 +46:35:59.9: 15.47 +/- 0.21 detection
Forced photometry on wcs_Lyn-03-Q1b1x1_2026-02-11_00-08-07_20.00sec_-14.90C_LIGHT_0233.fits at 06:46:21.44 +45:49:29.4: 15.07 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.28 +/- 0.12
Forced photometry filter REJECTED candidate at 07:00:35.33 +46:35:59.9: ref_mag=15.28 +/- 0.12 new_mean_mag=15.0132 delta=0.26 (need > 0.90)
Forced photometry reference-image weighted average: 15.13 +/- 0.11
Forced photometry filter REJECTED candidate at 06:46:21.44 +45:49:29.4: ref_mag=15.13 +/- 0.11 new_mean_mag=15.0667 delta=0.06 (need > 0.90)
Adding exclusion_list_local.txt__out129936.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 129715_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129715_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 129727_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129727_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 129729_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129729_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 129730_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129730_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 129733_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129733_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 129741_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129741_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 129751_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129751_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 129757_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129757_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 129760_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129760_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 129761_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129761_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 129762_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129762_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 129764_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129764_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 129767_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129767_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 129784_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129784_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 129789_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129789_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 129794_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129794_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:43:57.18 +43:15:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129795_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129795_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:31:43.84 +44:33:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129931_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129931_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:18:26.11 +49:26:10.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 129936_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
Preparing report for the candidate 129936_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
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Considering the candidate 129963_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129963_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:00:37.01 +42:05:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129981_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 129981_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:56:45.91 +44:40:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130000_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130000_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:46:43.60 +47:11:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130026_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130026_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130028_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130028_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:03:40.63 +44:53:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130040_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130040_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130059_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130059_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:01:59.37 +44:25:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130060_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130060_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:19:48.69 +45:07:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130061_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130061_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:05:47.48 +41:07:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130062_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130062_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:54:50.24 +42:57:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130076_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130076_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:57:17.62 +41:06:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130133_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130133_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130160_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130160_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:43:46.00 +42:38:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130164_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130164_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130170_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130170_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:03:51.75 +41:21:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130187_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130187_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:54:46.49 +41:34:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130192_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130192_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:27:24.17 +45:40:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130209_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130209_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:35:06.08 +42:12:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130233_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130233_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:15:56.16 +45:01:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130245_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130245_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130248_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130248_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:01:47.43 +48:22:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130250_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130250_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:00:27.96 +42:06:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130256_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130256_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:26:51.16 +44:27:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130257_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130257_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:21:50.88 +51:01:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130273_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130273_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:49:39.68 +44:03:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130276_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130276_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:42:08.26 +48:40:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130282_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130282_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:38:26.96 +44:19:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130289_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130289_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:14:22.06 +46:06:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130290_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130290_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:10:04.50 +46:51:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130310_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130310_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:57:11.35 +41:12:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130347_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130347_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:28:41.82 +48:11:28.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 130367_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130367_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:00:46.88 +47:57:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130380_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130380_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:49:20.01 +47:16:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130386_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130386_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:28:34.39 +47:02:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130389_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130389_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:01:47.46 +48:23:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130397_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130397_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:33:08.03 +43:20:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130425_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130425_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130429_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130429_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:00:21.03 +44:51:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130431_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130431_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:18:01.89 +48:16:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130445_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130445_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:27:30.01 +45:40:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130464_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130464_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:16:36.10 +48:54:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130484_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130484_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:15:47.09 +43:06:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130490_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130490_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:04:00.82 +47:01:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130510_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130510_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130523_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130523_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130563_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130563_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130566_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130566_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130569_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130569_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130595_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130595_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130597_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130597_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130705_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130705_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:13:32.16 +46:09:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130709_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130709_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130736_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130736_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 130739_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130739_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:02:24.94 +46:11:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130756_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130756_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 130768_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 130768_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
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Considering the candidate 61530_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 61530_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:55:21.10 +46:17:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120298_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 120298_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:26:02.68 +50:29:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104475_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 104475_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:57:09.07 +47:35:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95555_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 95555_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 06:49:38.59 +48:17:01.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 66275_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 66275_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:10:45.16 +47:02:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106552_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 106552_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks
**** FOUND 07:31:42.44 +47:33:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16850_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353
The candidate 16850_fd_Lyn-03-Q1b1x1_2026-10-07_02-21-03_20.00sec_-0.00C_LIGHTs_0353 did not pass the final checks