This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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 04 09.2946* 12 20 42.07 +29 20 44.2 14.3 U Com 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
ATO J185.1753+29.3458,2461139.7946,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J185.1753+29.3458 20260409.2946 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 04 09.2946* 12 19 41.24 +28 49 32.4 14.6 U Com 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
ATO J184.9220+28.8254,2461139.7946,14.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J184.9220+28.8254 20260409.2946 14.59CV 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
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 04 09.2946* 12 13 13.92 +28 50 10.8 14.5 U Com 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
ATO J183.3077+28.8358,2461139.7946,14.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J183.3077+28.8358 20260409.2946 14.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.84293929 27.02.2026 08:13:39.955 /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
First image: 2461098.84293929 27.02.2026 08:13:39.955 /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
Last image: 2461139.79497199 09.04.2026 07:04:35.580 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.96
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): 5454
Objects passed selection criteria: 5442
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 4039.75
Average stars matched: 3443.75 (85.2466 %)
Memory usage VmPeak: 110912 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 02:33:45 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: 2461098.84293929 27.02.2026 08:13:39.955 /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
First image: 2461098.84293929 27.02.2026 08:13:39.955 /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
Last image: 2461139.79497199 09.04.2026 07:04:35.580 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 37
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.71
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: 9 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): 21997
Objects passed selection criteria: 21936
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 17615.8
Average stars matched: 15739.8 (89.3504 %)
Memory usage VmPeak: 123904 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 02:34:28 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/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
SExtractor catalog cache: saved UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat to cache
SExtractor catalog cache: saved UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.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-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.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: 2461139.79427021
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits exists and is non-empty
Saving wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits to local_wcs_cache/
'wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits' -> 'local_wcs_cache/wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits'
wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits exists and is non-empty
Saving wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits to local_wcs_cache/
'wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits' -> 'local_wcs_cache/wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits'
wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits exists and is non-empty
Saving wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits to local_wcs_cache/
'wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits' -> 'local_wcs_cache/wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits'
wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits exists and is non-empty
Saving wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits to local_wcs_cache/
'wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits' -> 'local_wcs_cache/wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:00:24.339 +29:57:20.67
Second-epoch image center 12:00:12.062 +29:58:00.30
Angular distance between the image centers 0.0457 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:00:24.339 +29:57:20.67
Second-epoch image center 12:00:15.041 +29:58:28.29
Angular distance between the image centers 0.0385 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 12:00:12.062 +29:58:00.30
Second-epoch second image center 12:00:15.041 +29:58:28.29
Angular distance between the image centers 0.01327 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-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits &> /tmp/tmp.uMg7u05QwD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits &> /tmp/tmp.f6f2ioUvEf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits &> /tmp/tmp.dLOP1wECsT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits &> /tmp/tmp.7OsQks88CU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.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-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits and wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.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-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits and wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat
Found non-empty wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits and wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat
The reference image (wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits) and catalog (wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat) found
'wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat' -> 'wcsmag.cat'
Read 4543 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 170.7249 to 189.6721 deg, Dec +24.3968 to +35.1988 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 170.7249 to 189.6721 deg, Dec 24.3968 to 35.1988 deg
Loaded 3773 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): 2796 out of 2854 total matches.
Matched with Tycho-2 2854 out of 4543 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.971091
a=0.000000 b=1.000000 c=22.971091
From vast_summary.log: estimated ref. image limiting mag.: -7.96
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
2.4 pix UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
3.4 pix fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
3.5 pix fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
Limiting magnitude estimates:
15.0 mag. UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
15.0 mag. UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
15.0 mag. fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
15.0 mag. fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.uMg7u05QwD (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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.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-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits' -> 'wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
WCS_IMAGE_NAME=wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
WCS-calibrated image found: wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
Checking if the catalog wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat corresponding to the image wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits alredy exist and is non-empty...
Catalog wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat corresponding to the image wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
WCS catalog name: wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=286, passed=4543
Got 4543 stars (including 4251 good ones) from the SExtractor catalog wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat
util/solve_plate_with_UCAC5 got 4543 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 627 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4507 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 571 to 627 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits -region wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.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.f6f2ioUvEf (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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.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-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits' -> 'wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
WCS_IMAGE_NAME=wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
WCS-calibrated image found: wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
Checking if the catalog wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits.cat corresponding to the image wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits alredy exist and is non-empty...
Catalog wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits.cat corresponding to the image wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
WCS catalog name: wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=292, passed=4534
Got 4534 stars (including 4235 good ones) from the SExtractor catalog wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits.cat
util/solve_plate_with_UCAC5 got 4534 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 627 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 571 to 627 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits -region wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.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.dLOP1wECsT (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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
WCS_IMAGE_NAME=wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
WCS-calibrated image found: wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
Checking if the catalog wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits.cat corresponding to the image wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits.cat corresponding to the image wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
WCS catalog name: wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=535, passed=5699
Got 5699 stars (including 5159 good ones) from the SExtractor catalog wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits.cat
util/solve_plate_with_UCAC5 got 5699 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.7'
Seting catalog search parameters based on the expected field of view 936.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013010 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010408 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits -region wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.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.7OsQks88CU (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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
WCS_IMAGE_NAME=wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
WCS-calibrated image found: wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
Checking if the catalog wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat corresponding to the image wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat corresponding to the image wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
WCS catalog name: wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=615, passed=5733
Got 5733 stars (including 5117 good ones) from the SExtractor catalog wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat
util/solve_plate_with_UCAC5 got 5733 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.7'
Seting catalog search parameters based on the expected field of view 936.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013010 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010408 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 572 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 975 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits -region wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits'
Saving fully-calibrated image wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits'
Saving fully-calibrated image wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits'
Saving fully-calibrated image wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits'
Preparing the HTML report for the field UMa-14-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21031.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20933_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 20933_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 11:58:16.32 +32:17:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.214 4026743191046601344 179.56763230958 +32.29599177193 12.0020 11.4698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21031_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 21031_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 12:02:56.86 +26:59:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.750 4006823235807044608 180.73702889978 +26.99696050162 12.0966 11.4849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21043_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 21043_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 11:55:11.97 +32:25:45.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field UMa-14-Q2b1x1 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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
SExtractor catalog cache: saved UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat to cache
SExtractor catalog cache: saved UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.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-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
Creating symlink local_wcs_cache/wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.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-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits exists and is non-empty
wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits exists and is non-empty
wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits exists and is non-empty
wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:00:24.339 +29:57:20.67
Second-epoch image center 12:00:12.062 +29:58:00.30
Angular distance between the image centers 0.0457 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:00:24.339 +29:57:20.67
Second-epoch image center 12:00:15.041 +29:58:28.29
Angular distance between the image centers 0.0385 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 12:00:12.062 +29:58:00.30
Second-epoch second image center 12:00:15.041 +29:58:28.29
Angular distance between the image centers 0.01327 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-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits &> /tmp/tmp.5MUf1KBQUu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits &> /tmp/tmp.SFD49mbH5t
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits &> /tmp/tmp.Y0krdHEPyb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits &> /tmp/tmp.PcPYLEZ7j8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.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-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits and wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.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-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits and wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat
Found non-empty wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits and wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat
The reference image (wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits) and catalog (wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat) found
'wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat' -> 'wcsmag.cat'
Read 21628 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 170.6653 to 189.6720 deg, Dec +24.3960 to +35.2243 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 170.6653 to 189.6720 deg, Dec 24.3960 to 35.2243 deg
Loaded 3794 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): 2800 out of 2949 total matches.
Matched with Tycho-2 2949 out of 21628 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.849551
a=0.000000 b=1.000000 c=22.849551
From vast_summary.log: estimated ref. image limiting mag.: -7.71
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.14
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.14
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 17 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
2.4 pix UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
3.3 pix fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
3.2 pix fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
Limiting magnitude estimates:
15.1 mag. UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
15.1 mag. UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
15.1 mag. fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
15.2 mag. fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5MUf1KBQUu (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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.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-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits' -> 'wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
WCS_IMAGE_NAME=wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
WCS-calibrated image found: wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
Checking if the catalog wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat corresponding to the image wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits alredy exist and is non-empty...
Catalog wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat corresponding to the image wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
WCS catalog name: wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=852, passed=21624
Got 21624 stars (including 20742 good ones) from the SExtractor catalog wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat
util/solve_plate_with_UCAC5 got 21624 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 21536 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 571 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 21533 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 21533 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits -region wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.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.SFD49mbH5t (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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.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-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits' -> 'wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
WCS_IMAGE_NAME=wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
WCS-calibrated image found: wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
Checking if the catalog wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits.cat corresponding to the image wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits alredy exist and is non-empty...
Catalog wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits.cat corresponding to the image wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
WCS catalog name: wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=856, passed=21614
Got 21614 stars (including 20730 good ones) from the SExtractor catalog wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits.cat
util/solve_plate_with_UCAC5 got 21614 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 21526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 571 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 21527 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 21527 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits -region wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.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.Y0krdHEPyb (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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
WCS_IMAGE_NAME=wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
WCS-calibrated image found: wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
Checking if the catalog wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits.cat corresponding to the image wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits.cat corresponding to the image wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
WCS catalog name: wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=2242, passed=21351
Got 21351 stars (including 19093 good ones) from the SExtractor catalog wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits.cat
util/solve_plate_with_UCAC5 got 21351 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.7'
Seting catalog search parameters based on the expected field of view 936.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013010 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010408 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 20849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 572 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 20850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 20850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits -region wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.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.PcPYLEZ7j8 (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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
WCS_IMAGE_NAME=wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
WCS-calibrated image found: wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
Checking if the catalog wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat corresponding to the image wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat corresponding to the image wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
WCS catalog name: wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2489, passed=21860
Got 21860 stars (including 19354 good ones) from the SExtractor catalog wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat
util/solve_plate_with_UCAC5 got 21860 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.7'
Seting catalog search parameters based on the expected field of view 936.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013010 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010408 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 20780 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.2)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 20779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 20779 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits -region wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/wcs_UMa-14-Q2b1x1_2026-02-27_02-13-39_20.00sec_-14.90C_LIGHT_0096.fits
Saving fully-calibrated image wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/wcs_UMa-14-Q2b1x1_2026-02-27_02-14-25_20.00sec_-15.00C_LIGHT_0097.fits
Saving fully-calibrated image wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-03-34_20.00sec_-5.00C_LIGHT_0254.fits
Saving fully-calibrated image wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.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_2026-04-09_CI_UMa-14-Q2b1x1_023132_TTUQ2b1x1_24220_mtEPXtU2/wcs_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255.fits
Preparing the HTML report for the field UMa-14-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out31325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35150.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out36008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out35716.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out34462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35426.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 31325_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 31325_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 11:42:32.57 +25:44:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 3.255 4005379748838126720 175.63636392317 +25.73364853947 13.8175 13.1118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32377_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 32377_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 12:19:28.22 +26:36:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34274_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 34274_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 12:17:48.33 +26:01:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34462_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
Preparing report for the candidate 34462_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
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Considering the candidate 34705_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 34705_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 12:12:34.07 +30:48:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.665 4014459618939954176 183.14168303666 +30.80054683085 15.0111 14.6801 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34762_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 34762_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 12:20:04.79 +27:58:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35094_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 35094_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 12:06:24.04 +25:50:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 0.447 4003507383615418112 181.60007434468 +25.84674095938 14.5407 14.0466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35150_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 35150_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 12:08:37.74 +27:18:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 2.300 4006714281076572672 182.15654509341 +27.30245961446 14.8105 14.2208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35221_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 35221_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 12:00:26.06 +26:20:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35379_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
Preparing report for the candidate 35379_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
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Considering the candidate 35426_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
Preparing report for the candidate 35426_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
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Considering the candidate 35518_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 35518_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 12:04:58.96 +32:23:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35553_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 35553_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 11:59:29.37 +28:06:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35571_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 35571_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 12:04:11.87 +26:43:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 0.964 4006613332165434496 181.04966878572 +26.72227388690 14.8324 14.1464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.964#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35643_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 35643_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 11:57:39.58 +26:22:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 1.372 4006355874646024320 179.41507565741 +26.37470193554 14.6783 13.9107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35716_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 35716_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks
**** FOUND 12:05:45.48 +31:04:45.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)
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Considering the candidate 36008_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255
The candidate 36008_fd_UMa-14-Q2b1x1_2026-04-09_02-04-35_20.00sec_-5.00C_LIGHT_0255 did not pass the final checks