This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1
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 05 15.3634 2461175.8634 12.79 10:38:18.03 +62:46:30.7
145.07358 48.23068 galactic UMa Second-epoch detections are separated by 0.8" and 3.0 pix
The object was found in VSX 2" Gaia DR3 1049258728002278528
Type: L
# Max. Min./Amp. JD0 Period
12.620 G 13.560 G M
The object was not found in astcheck.
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits at 10:38:18.03 +62:46:30.7: 13.73 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:38:18.03 +62:46:30.7: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 15.3634* 10 38 18.03 +62 46 30.7 12.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1049258728002278528,2461175.8634,12.79,0.05,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
Gaia DR3 1049258728002278528 20260515.3634 12.79CV 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 05 15.3634 2461175.8634 13.34 10:10:05.84 +62:39:54.6
148.15319 45.77348 galactic UMa Second-epoch detections are separated by 0.3" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 10:10:05.84 +62:39:54.6 (user input) | T | P | (position from user input) J-Ks=0.711+/-0.033 (K)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits at 10:10:05.84 +62:39:54.6: 14.23 +/- 0.06 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:10:05.84 +62:39:54.6: 14.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 15.3634* 10 10 05.84 +62 39 54.6 13.3 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461175.8634,13.34,0.05,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
target 20260515.3634 13.34CV 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: 2461082.80532322 11.02.2026 07:19:29.926 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
First image: 2461082.80532322 11.02.2026 07:19:29.926 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
Last image: 2461175.86366917 15.05.2026 08:43:31.016 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 7379
Objects passed selection criteria: 7337
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 4798
Average stars matched: 4623.5 (96.3631 %)
Memory usage VmPeak: 113152 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri May 15 06:34:28 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: 2461082.80532322 11.02.2026 07:19:29.926 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
First image: 2461082.80532322 11.02.2026 07:19:29.926 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
Last image: 2461175.86366917 15.05.2026 08:43:31.016 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 22
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.23
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 11 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 39886
Objects passed selection criteria: 39735
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 25985
Average stars matched: 24921.2 (95.9063 %)
Memory usage VmPeak: 141776 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri May 15 06:35:56 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 --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
SExtractor catalog cache: saved UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat to cache
SExtractor catalog cache: saved UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.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/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461175.86320646
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits exists and is non-empty
Saving wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits to local_wcs_cache/
'wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits' -> 'local_wcs_cache/wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits'
wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits exists and is non-empty
Saving wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits to local_wcs_cache/
'wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits' -> 'local_wcs_cache/wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits'
wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits exists and is non-empty
Saving wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits to local_wcs_cache/
'wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits' -> 'local_wcs_cache/wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits'
wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits exists and is non-empty
Saving wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits to local_wcs_cache/
'wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits' -> 'local_wcs_cache/wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits (1st reference image)
verification OK: wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
Image size: 941.6'x627.1' 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: 10:17:03.928 +61:59:42.80 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_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits (1st new image)
verification OK: wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
Image size: 941.7'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: 10:17:07.045 +61:59:34.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:17:03.928 +61:59:42.80
Second-epoch image center 10:17:07.045 +61:59:34.21
Angular distance between the image centers 0.0065 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits (2nd new image)
verification OK: wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
Image size: 941.7'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: 10:17:09.637 +61:59:26.74 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:17:03.928 +61:59:42.80
Second-epoch image center 10:17:09.637 +61:59:26.74
Angular distance between the image centers 0.0120 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 10:17:07.045 +61:59:34.21
Second-epoch second image center 10:17:09.637 +61:59:26.74
Angular distance between the image centers 0.00548 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits &> /tmp/tmp.OypB1WOjy9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits &> /tmp/tmp.2X5yk6h0OS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits &> /tmp/tmp.ETbSmZJBwH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits &> /tmp/tmp.DC48BYVR7S
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.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_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits and wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat
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_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits and wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat
Found non-empty wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits and wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat
The reference image (wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits) and catalog (wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat) found
'wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat' -> 'wcsmag.cat'
Read 7643 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 134.1814 to 172.7540 deg, Dec +55.2234 to +67.4791 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 134.1814 to 172.7540 deg, Dec 55.2234 to 67.4791 deg
Loaded 7304 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): 4370 out of 4605 total matches.
Matched with Tycho-2 4605 out of 7643 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.870750
a=0.000000 b=1.000000 c=22.870750
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7643 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 134.1814 to 172.7540 deg, Dec +55.2234 to +67.4791 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 134.1814 to 172.7540 deg, Dec 55.2234 to 67.4791 deg
Loaded 7304 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): 4370 out of 4605 total matches.
Matched with Tycho-2 4605 out of 7643 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits:
Forced-photometry filter: calibrated wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits -> calib.txt_param_ref_wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits (aperture=6.2)
Read 7662 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 134.1813 to 172.7538 deg, Dec +55.2234 to +67.4798 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 134.1813 to 172.7538 deg, Dec 55.2234 to 67.4798 deg
Loaded 7305 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): 4361 out of 4610 total matches.
Matched with Tycho-2 4610 out of 7662 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits:
Forced-photometry filter: calibrated wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits -> calib.txt_param_ref_wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
2.1 pix UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
3.3 pix fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
3.3 pix fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
2.1 pix wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
2.1 pix wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
Limiting magnitude estimates:
15.4 mag. UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
15.4 mag. UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
13.7 mag. fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
13.5 mag. fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.OypB1WOjy9 (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_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits' -> 'wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
WCS_IMAGE_NAME=wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
WCS-calibrated image found: wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
Checking if the catalog wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat corresponding to the image wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits alredy exist and is non-empty...
Catalog wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat corresponding to the image wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
WCS catalog name: wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=549, passed=7643
Got 7643 stars (including 7078 good ones) from the SExtractor catalog wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat
util/solve_plate_with_UCAC5 got 7643 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 7551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 7551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 7551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits N_match=978 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.473 sigma_q2_arcsec=0.349 sigma_q3_arcsec=0.366 sigma_q4_arcsec=0.304 n_q1=236 n_q2=225 n_q3=242 n_q4=275 worst_quadrant_to_overall_ratio=1.317
The image catalog is written to wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits -region wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2X5yk6h0OS (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_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits' -> 'wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
WCS_IMAGE_NAME=wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
WCS-calibrated image found: wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
Checking if the catalog wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat corresponding to the image wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits alredy exist and is non-empty...
Catalog wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat corresponding to the image wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
WCS catalog name: wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=562, passed=7662
Got 7662 stars (including 7088 good ones) from the SExtractor catalog wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat
util/solve_plate_with_UCAC5 got 7662 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 7579 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 7579 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 7579 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits N_match=978 sigma_overall_arcsec=0.383 sigma_q1_arcsec=0.521 sigma_q2_arcsec=0.377 sigma_q3_arcsec=0.383 sigma_q4_arcsec=0.302 n_q1=229 n_q2=228 n_q3=238 n_q4=283 worst_quadrant_to_overall_ratio=1.359
The image catalog is written to wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits -region wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ETbSmZJBwH (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_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.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_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
WCS_IMAGE_NAME=wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
WCS-calibrated image found: wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
Checking if the catalog wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat corresponding to the image wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat corresponding to the image wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
WCS catalog name: wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=68, passed=2259
Got 2259 stars (including 2190 good ones) from the SExtractor catalog wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat
util/solve_plate_with_UCAC5 got 2259 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
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 2191 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
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 2190 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 2190 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits N_match=980 sigma_overall_arcsec=0.346 sigma_q1_arcsec=0.285 sigma_q2_arcsec=0.403 sigma_q3_arcsec=0.315 sigma_q4_arcsec=0.444 n_q1=249 n_q2=361 n_q3=303 n_q4=67 worst_quadrant_to_overall_ratio=1.284
The image catalog is written to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits -region wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.DC48BYVR7S (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_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.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_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
WCS_IMAGE_NAME=wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
WCS-calibrated image found: wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
Checking if the catalog wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat corresponding to the image wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat corresponding to the image wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
WCS catalog name: wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=61, passed=1758
Got 1758 stars (including 1696 good ones) from the SExtractor catalog wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat
util/solve_plate_with_UCAC5 got 1758 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
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 1684 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
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 1682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 1682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits N_match=977 sigma_overall_arcsec=0.318 sigma_q1_arcsec=0.289 sigma_q2_arcsec=0.346 sigma_q3_arcsec=0.328 sigma_q4_arcsec=0.440 n_q1=250 n_q2=358 n_q3=310 n_q4=59 worst_quadrant_to_overall_ratio=1.384
The image catalog is written to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits -region wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits sigma_overall=0.360 worst_q_ratio=1.317
ref2=UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits sigma_overall=0.383 worst_q_ratio=1.359
new1=fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits sigma_overall=0.346 worst_q_ratio=1.284
new2=fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits sigma_overall=0.318 worst_q_ratio=1.384
reference average sigma_overall=0.3715 worst_q_ratio=1.338
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304_astrometric_residuals.png (978 matched stars from wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305_astrometric_residuals.png (978 matched stars from wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140_astrometric_residuals.png (980 matched stars from wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141_astrometric_residuals.png (977 matched stars from wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits'
Saving fully-calibrated image wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits'
Preparing the HTML report for the field UMa-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field UMa-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
SExtractor catalog cache: saved UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat to cache
SExtractor catalog cache: saved UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
Creating symlink local_wcs_cache/wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits exists and is non-empty
wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits exists and is non-empty
wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits exists and is non-empty
wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits (1st reference image)
verification OK: wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
Image size: 941.6'x627.1' 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: 10:17:03.928 +61:59:42.80 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_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits (1st new image)
verification OK: wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
Image size: 941.7'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: 10:17:07.045 +61:59:34.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:17:03.928 +61:59:42.80
Second-epoch image center 10:17:07.045 +61:59:34.21
Angular distance between the image centers 0.0065 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits (2nd new image)
verification OK: wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
Image size: 941.7'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: 10:17:09.637 +61:59:26.74 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:17:03.928 +61:59:42.80
Second-epoch image center 10:17:09.637 +61:59:26.74
Angular distance between the image centers 0.0120 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 10:17:07.045 +61:59:34.21
Second-epoch second image center 10:17:09.637 +61:59:26.74
Angular distance between the image centers 0.00548 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits &> /tmp/tmp.aNfBiXRB2A
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits &> /tmp/tmp.4BTH6ZD4Nh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits &> /tmp/tmp.LXc4jTXWAT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits &> /tmp/tmp.UaxZVlKgEu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.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_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits and wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat
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_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits and wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat
Found non-empty wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits and wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat
The reference image (wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits) and catalog (wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat) found
'wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat' -> 'wcsmag.cat'
Read 42264 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 134.1815 to 172.8776 deg, Dec +55.2077 to +67.4859 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 134.1815 to 172.8776 deg, Dec 55.2077 to 67.4859 deg
Loaded 7342 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): 4155 out of 4668 total matches.
Matched with Tycho-2 4668 out of 42264 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.756400
a=0.000000 b=1.000000 c=22.756400
From vast_summary.log: estimated ref. image limiting mag.: -7.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.53
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 42264 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 134.1815 to 172.8776 deg, Dec +55.2077 to +67.4859 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 134.1815 to 172.8776 deg, Dec 55.2077 to 67.4859 deg
Loaded 7342 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): 4155 out of 4668 total matches.
Matched with Tycho-2 4668 out of 42264 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits:
Forced-photometry filter: calibrated wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits -> calib.txt_param_ref_wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits (aperture=4.8)
Read 42564 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 134.1813 to 172.8782 deg, Dec +55.2076 to +67.4899 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 134.1813 to 172.8782 deg, Dec 55.2076 to 67.4899 deg
Loaded 7342 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): 4153 out of 4662 total matches.
Matched with Tycho-2 4662 out of 42564 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits:
Forced-photometry filter: calibrated wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits -> calib.txt_param_ref_wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 22 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
1.9 pix UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
3.2 pix fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
3.2 pix fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
1.9 pix wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
1.9 pix wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
Limiting magnitude estimates:
15.5 mag. UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
15.5 mag. UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
14.0 mag. fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
14.0 mag. fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.5 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.aNfBiXRB2A (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_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits' -> 'wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
WCS_IMAGE_NAME=wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
WCS-calibrated image found: wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
Checking if the catalog wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat corresponding to the image wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits alredy exist and is non-empty...
Catalog wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat corresponding to the image wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits
WCS catalog name: wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=1963, passed=42243
Got 42243 stars (including 40203 good ones) from the SExtractor catalog wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat
util/solve_plate_with_UCAC5 got 42243 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 977 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 41746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 41748 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 41748 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 982 stars left (next iteration limit 1080)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits N_match=982 sigma_overall_arcsec=0.346 sigma_q1_arcsec=0.480 sigma_q2_arcsec=0.338 sigma_q3_arcsec=0.335 sigma_q4_arcsec=0.290 n_q1=235 n_q2=225 n_q3=245 n_q4=277 worst_quadrant_to_overall_ratio=1.390
The image catalog is written to wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits -region wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4BTH6ZD4Nh (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_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits' -> 'wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
WCS_IMAGE_NAME=wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
WCS-calibrated image found: wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
Checking if the catalog wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat corresponding to the image wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits alredy exist and is non-empty...
Catalog wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat corresponding to the image wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits
WCS catalog name: wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1976, passed=42549
Got 42549 stars (including 40495 good ones) from the SExtractor catalog wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat
util/solve_plate_with_UCAC5 got 42549 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 41998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 41997 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 41997 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits N_match=980 sigma_overall_arcsec=0.365 sigma_q1_arcsec=0.501 sigma_q2_arcsec=0.359 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.307 n_q1=232 n_q2=223 n_q3=242 n_q4=283 worst_quadrant_to_overall_ratio=1.371
The image catalog is written to wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits -region wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LXc4jTXWAT (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_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.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_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
WCS_IMAGE_NAME=wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
WCS-calibrated image found: wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
Checking if the catalog wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat corresponding to the image wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat corresponding to the image wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
WCS catalog name: wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=285, passed=11030
Got 11030 stars (including 10727 good ones) from the SExtractor catalog wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat
util/solve_plate_with_UCAC5 got 11030 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
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 10639 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
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 10639 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 10639 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits N_match=980 sigma_overall_arcsec=0.349 sigma_q1_arcsec=0.290 sigma_q2_arcsec=0.407 sigma_q3_arcsec=0.326 sigma_q4_arcsec=0.457 n_q1=247 n_q2=360 n_q3=305 n_q4=68 worst_quadrant_to_overall_ratio=1.312
The image catalog is written to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits -region wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.UaxZVlKgEu (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_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.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_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
WCS_IMAGE_NAME=wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
WCS-calibrated image found: wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
Checking if the catalog wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat corresponding to the image wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat corresponding to the image wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
WCS catalog name: wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=229, passed=8873
Got 8873 stars (including 8637 good ones) from the SExtractor catalog wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat
util/solve_plate_with_UCAC5 got 8873 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
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 8569 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
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 8567 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 8567 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits N_match=977 sigma_overall_arcsec=0.324 sigma_q1_arcsec=0.282 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.313 sigma_q4_arcsec=0.445 n_q1=249 n_q2=352 n_q3=316 n_q4=60 worst_quadrant_to_overall_ratio=1.372
The image catalog is written to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits -region wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.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_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-42-51_20.00sec_-4.90C_LIGHTs_0140.fits
Saving fully-calibrated image wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.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_2026-05-15_CI_UMa-03-Q1b1x1_041510_TTUQ1b1x1_909506_locG3zM1/wcs_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141.fits
Preparing the HTML report for the field UMa-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits at 10:01:25.10 +64:40:34.7: 13.76 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:01:25.10 +64:40:34.7: 13.82 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits at 10:06:01.24 +64:46:01.0: 14.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.03
Forced photometry filter REJECTED candidate at 10:01:25.10 +64:40:34.7: ref_mag=13.79 +/- 0.03 new_mean_mag=13.2517 delta=0.54 (need > 0.90)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits at 10:04:54.15 +66:20:30.0: 14.15 +/- 0.06 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits at 10:38:18.03 +62:46:30.7: 13.73 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits at 10:47:19.69 +60:47:43.2: 13.13 +/- 0.02 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-19-29_20.00sec_-15.00C_LIGHT_0304.fits at 10:10:05.84 +62:39:54.6: 14.23 +/- 0.06 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:06:01.24 +64:46:01.0: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.04
Forced photometry filter REJECTED candidate at 10:06:01.24 +64:46:01.0: ref_mag=14.22 +/- 0.04 new_mean_mag=13.3283 delta=0.89 (need > 0.90)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:04:54.15 +66:20:30.0: 14.34 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.04
Forced photometry filter REJECTED candidate at 10:04:54.15 +66:20:30.0: ref_mag=14.23 +/- 0.04 new_mean_mag=13.3721 delta=0.86 (need > 0.90)
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:38:18.03 +62:46:30.7: 13.69 +/- 0.04 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:10:05.84 +62:39:54.6: 14.18 +/- 0.06 detection
Forced photometry on wcs_UMa-03-Q1b1x1_2026-02-11_01-20-06_20.00sec_-15.00C_LIGHT_0305.fits at 10:47:19.69 +60:47:43.2: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry reference-image weighted average: 14.20 +/- 0.04
Forced photometry filter KEPT candidate at 10:38:18.03 +62:46:30.7: ref_mag=13.71 +/- 0.03 new_mean_mag=12.7776 delta=0.94 (need > 0.90)
Forced photometry filter KEPT candidate at 10:10:05.84 +62:39:54.6: ref_mag=14.20 +/- 0.04 new_mean_mag=13.2982 delta=0.91 (need > 0.90)
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter REJECTED candidate at 10:47:19.69 +60:47:43.2: ref_mag=13.15 +/- 0.02 new_mean_mag=12.4894 delta=0.66 (need > 0.90)
Adding exclusion_list_local.txt__out22733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23501.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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 53039_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53039_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
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Considering the candidate 53188_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53188_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 53259_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53259_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 53293_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53293_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 53313_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53313_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 53425_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53425_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 53475_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53475_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 53569_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53569_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 53591_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53591_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 53673_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53673_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 53748_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53748_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 53753_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53753_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
**** FOUND 10:07:01.50 +66:17:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53768_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53768_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
**** FOUND 10:36:04.01 +63:36:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53804_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53804_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 53809_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53809_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 53945_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53945_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 53950_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 53950_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 37059_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 37059_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
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Considering the candidate 27736_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 27736_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks
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Considering the candidate 22733_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
Preparing report for the candidate 22733_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
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Considering the candidate 23501_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
Preparing report for the candidate 23501_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
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Considering the candidate 14419_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141
The candidate 14419_fd_UMa-03-Q1b1x1_2026-05-15_03-43-31_20.00sec_-5.00C_LIGHTs_0141 did not pass the final checks