This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 02.1256 2461193.6256 14.56 09:53:36.85 +44:40:43.6
174.55760 50.56334 galactic UMa Second-epoch detections are separated by 8.5" and 0.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:53:36.85 +44:40:43.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits at 09:53:36.85 +44:40:43.6: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits at 09:53:36.85 +44:40:43.6: 16.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 02.1256* 09 53 36.85 +44 40 43.6 14.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461193.6256,14.56,0.05,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
target 20260602.1256 14.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 02.1256 2461193.6256 14.54 09:37:04.53 +43:21:45.1
177.23278 47.82184 galactic UMa Second-epoch detections are separated by 6.3" and 0.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:37:04.53 +43:21:45.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits at 09:37:04.53 +43:21:45.1: 16.31 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits at 09:37:04.53 +43:21:45.1: 16.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 02.1256* 09 37 04.53 +43 21 45.1 14.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461193.6256,14.54,0.05,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
target 20260602.1256 14.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 02.1256 2461193.6256 14.52 09:28:41.82 +41:43:39.1
179.80792 46.41323 galactic UMa Second-epoch detections are separated by 7.7" and 0.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:28:41.82 +41:43:39.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits at 09:28:41.82 +41:43:39.1: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits at 09:28:41.82 +41:43:39.1: 16.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 02.1256* 09 28 41.82 +41 43 39.1 14.5 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461193.6256,14.52,0.05,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
target 20260602.1256 14.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 02.1256 2461193.6256 14.43 09:24:17.47 +42:02:20.1
179.41547 45.57951 galactic UMa Second-epoch detections are separated by 7.7" and 0.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 09:24:17.47 +42:02:20.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits at 09:24:17.47 +42:02:20.1: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits at 09:24:17.47 +42:02:20.1: 16.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 02.1256* 09 24 17.47 +42 02 20.1 14.4 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461193.6256,14.43,0.05,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
target 20260602.1256 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 02.1256 2461193.6256 13.71 09:12:28.62 +42:19:07.2
179.10786 43.38402 galactic Lyn Second-epoch detections are separated by 1.2" and 1.5 pix
The object was found in VSX 0" Mis V1406
Type: SR
# Max. Min./Amp. JD0 Period
13.900 CV Y 0.680 CV 86.742588000000
The object was not found in astcheck.
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits at 09:12:28.62 +42:19:07.2: 14.71 +/- 0.09 detection
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits at 09:12:28.62 +42:19:07.2: 14.74 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V1406,2461193.6256,13.71,0.05,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
Mis V1406 20260602.1256 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.82250781 18.01.2026 07:44:14.675 /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
First image: 2461058.82250781 18.01.2026 07:44:14.675 /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
Last image: 2461193.62582690 02.06.2026 03:01:01.444 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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): 6913
Objects passed selection criteria: 6888
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 4846.75
Average stars matched: 4528.5 (93.4337 %)
Memory usage VmPeak: 112632 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 1 15:05:05 CDT 2026
VaST build number 1.0rc89-85-g6dfb2809
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 1 22:07:50 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.82250781 18.01.2026 07:44:14.675 /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
First image: 2461058.82250781 18.01.2026 07:44:14.675 /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
Last image: 2461193.62582690 02.06.2026 03:01:01.444 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 80
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.14
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: 12 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): 38549
Objects passed selection criteria: 38433
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 28385.2
Average stars matched: 26376 (92.9215 %)
Memory usage VmPeak: 138820 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 1 15:05:05 CDT 2026
VaST build number 1.0rc89-85-g6dfb2809
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 1 22:09:15 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-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
SExtractor catalog cache: saved UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat to cache
SExtractor catalog cache: saved UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.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-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.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: 2461193.62540978
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits exists and is non-empty
Saving wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits to local_wcs_cache/
'wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits' -> 'local_wcs_cache/wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits'
wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits exists and is non-empty
Saving wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits to local_wcs_cache/
'wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits' -> 'local_wcs_cache/wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits'
wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits exists and is non-empty
Saving wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits to local_wcs_cache/
'wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits' -> 'local_wcs_cache/wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits'
wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits exists and is non-empty
Saving wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits to local_wcs_cache/
'wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits' -> 'local_wcs_cache/wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits (1st reference image)
verification OK: wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:36:00.662 +46:00:08.08 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits (1st new image)
verification OK: wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:36:02.979 +46:01:36.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:36:00.662 +46:00:08.08
Second-epoch image center 09:36:02.979 +46:01:36.08
Angular distance between the image centers 0.0253 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits (2nd new image)
verification OK: wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:36:02.324 +46:01:42.05 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:36:00.662 +46:00:08.08
Second-epoch image center 09:36:02.324 +46:01:42.05
Angular distance between the image centers 0.0265 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 09:36:02.979 +46:01:36.08
Second-epoch second image center 09:36:02.324 +46:01:42.05
Angular distance between the image centers 0.00252 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-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits &> /tmp/tmp.2Xk5cbHI0W
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits &> /tmp/tmp.BP7vVu3t3w
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits &> /tmp/tmp.gBw0KKgcLU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits &> /tmp/tmp.LyG8RAnMXH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.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-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits and wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits and wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat
Found non-empty wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits and wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat
The reference image (wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits) and catalog (wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat) found
'wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat' -> 'wcsmag.cat'
Read 8167 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 131.3127 to 155.8106 deg, Dec +39.8609 to +51.4112 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 131.3127 to 155.8106 deg, Dec 39.8609 to 51.4112 deg
Loaded 5369 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): 3785 out of 3992 total matches.
Matched with Tycho-2 3992 out of 8167 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.900300
a=0.000000 b=1.000000 c=22.900300
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8167 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 131.3127 to 155.8106 deg, Dec +39.8609 to +51.4112 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 131.3127 to 155.8106 deg, Dec 39.8609 to 51.4112 deg
Loaded 5369 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): 3785 out of 3992 total matches.
Matched with Tycho-2 3992 out of 8167 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits:
Forced-photometry filter: calibrated wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits -> calib.txt_param_ref_wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits (aperture=6.1)
Read 8217 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 131.3128 to 155.8106 deg, Dec +39.8864 to +51.4195 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 131.3128 to 155.8106 deg, Dec 39.8864 to 51.4195 deg
Loaded 5366 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): 3787 out of 3997 total matches.
Matched with Tycho-2 3997 out of 8217 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits:
Forced-photometry filter: calibrated wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits -> calib.txt_param_ref_wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
2.1 pix UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
2.4 pix fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
2.4 pix fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
2.1 pix wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
2.1 pix wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
Limiting magnitude estimates:
15.5 mag. UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
15.5 mag. UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
14.5 mag. fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
14.5 mag. fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.6 (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.2Xk5cbHI0W (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.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-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits' -> 'wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
WCS_IMAGE_NAME=wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
WCS-calibrated image found: wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
Checking if the catalog wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat corresponding to the image wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits alredy exist and is non-empty...
Catalog wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat corresponding to the image wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
WCS catalog name: wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=568, passed=8167
Got 8167 stars (including 7592 good ones) from the SExtractor catalog wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat
util/solve_plate_with_UCAC5 got 8167 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.9 to 51.4)
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: 975 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 8079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 649 to 709 (Dec 39.9 to 51.4)
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(), 8081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 8081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits N_match=975 sigma_overall_arcsec=0.368 sigma_q1_arcsec=0.465 sigma_q2_arcsec=0.376 sigma_q3_arcsec=0.329 sigma_q4_arcsec=0.329 n_q1=213 n_q2=265 n_q3=256 n_q4=241 worst_quadrant_to_overall_ratio=1.265
The image catalog is written to wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits -region wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.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.BP7vVu3t3w (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.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-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits' -> 'wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
WCS_IMAGE_NAME=wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
WCS-calibrated image found: wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
Checking if the catalog wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat corresponding to the image wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits alredy exist and is non-empty...
Catalog wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat corresponding to the image wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
WCS catalog name: wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=561, passed=8217
Got 8217 stars (including 7647 good ones) from the SExtractor catalog wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat
util/solve_plate_with_UCAC5 got 8217 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.9 to 51.4)
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: 975 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 8160 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.9 to 51.4)
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(), 8159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 8159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits N_match=975 sigma_overall_arcsec=0.361 sigma_q1_arcsec=0.453 sigma_q2_arcsec=0.380 sigma_q3_arcsec=0.362 sigma_q4_arcsec=0.294 n_q1=208 n_q2=264 n_q3=262 n_q4=241 worst_quadrant_to_overall_ratio=1.254
The image catalog is written to wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits -region wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.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.gBw0KKgcLU (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_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.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_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
WCS_IMAGE_NAME=wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
WCS-calibrated image found: wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
Checking if the catalog wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat corresponding to the image wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat corresponding to the image wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
WCS catalog name: wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=306, passed=4453
Got 4453 stars (including 4143 good ones) from the SExtractor catalog wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat
util/solve_plate_with_UCAC5 got 4453 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 651 to 708 (Dec 40.4 to 51.3)
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: 975 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 4390 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 651 to 708 (Dec 40.4 to 51.3)
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(), 4390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 4390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits N_match=975 sigma_overall_arcsec=0.453 sigma_q1_arcsec=0.315 sigma_q2_arcsec=0.512 sigma_q3_arcsec=0.430 sigma_q4_arcsec=0.614 n_q1=222 n_q2=281 n_q3=232 n_q4=240 worst_quadrant_to_overall_ratio=1.354
The image catalog is written to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits -region wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.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.LyG8RAnMXH (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_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.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_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
WCS_IMAGE_NAME=wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
WCS-calibrated image found: wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
Checking if the catalog wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat corresponding to the image wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat corresponding to the image wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
WCS catalog name: wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=313, passed=4486
Got 4486 stars (including 4167 good ones) from the SExtractor catalog wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat
util/solve_plate_with_UCAC5 got 4486 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 651 to 708 (Dec 40.4 to 51.3)
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(), 962 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(), 4409 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 651 to 708 (Dec 40.4 to 51.3)
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(), 4410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 4411 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits N_match=974 sigma_overall_arcsec=0.464 sigma_q1_arcsec=0.348 sigma_q2_arcsec=0.518 sigma_q3_arcsec=0.455 sigma_q4_arcsec=0.579 n_q1=228 n_q2=276 n_q3=229 n_q4=241 worst_quadrant_to_overall_ratio=1.246
The image catalog is written to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits -region wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits sigma_overall=0.368 worst_q_ratio=1.265
ref2=UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits sigma_overall=0.361 worst_q_ratio=1.254
new1=fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits sigma_overall=0.453 worst_q_ratio=1.354
new2=fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits sigma_overall=0.464 worst_q_ratio=1.246
reference average sigma_overall=0.3645 worst_q_ratio=1.2595
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332_astrometric_residuals.png (975 matched stars from wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333_astrometric_residuals.png (975 matched stars from wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023_astrometric_residuals.png (975 matched stars from wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024_astrometric_residuals.png (974 matched stars from wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits'
Saving fully-calibrated image wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits'
Preparing the HTML report for the field UMa-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field UMa-09-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-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
SExtractor catalog cache: saved UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat to cache
SExtractor catalog cache: saved UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.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-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
Creating symlink local_wcs_cache/wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.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-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits exists and is non-empty
wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits exists and is non-empty
wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits exists and is non-empty
wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits (1st reference image)
verification OK: wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:36:00.662 +46:00:08.08 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits (1st new image)
verification OK: wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:36:02.979 +46:01:36.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:36:00.662 +46:00:08.08
Second-epoch image center 09:36:02.979 +46:01:36.08
Angular distance between the image centers 0.0253 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits (2nd new image)
verification OK: wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
Image size: 937.1'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:36:02.324 +46:01:42.05 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:36:00.662 +46:00:08.08
Second-epoch image center 09:36:02.324 +46:01:42.05
Angular distance between the image centers 0.0265 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 09:36:02.979 +46:01:36.08
Second-epoch second image center 09:36:02.324 +46:01:42.05
Angular distance between the image centers 0.00252 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-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits &> /tmp/tmp.J84s5Nos8V
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits &> /tmp/tmp.kWWlpmizf0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits &> /tmp/tmp.kbEzKVwPzW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits &> /tmp/tmp.cRtC329m9U
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.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-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits and wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits and wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat
Found non-empty wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits and wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat
The reference image (wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits) and catalog (wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat) found
'wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat' -> 'wcsmag.cat'
Read 43830 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 131.1885 to 155.9231 deg, Dec +39.8074 to +51.4128 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 131.1885 to 155.9231 deg, Dec 39.8074 to 51.4128 deg
Loaded 5468 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): 3562 out of 4004 total matches.
Matched with Tycho-2 4004 out of 43830 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.793550
a=0.000000 b=1.000000 c=22.793550
From vast_summary.log: estimated ref. image limiting mag.: -7.14
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.65
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.65
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 43830 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 131.1885 to 155.9231 deg, Dec +39.8074 to +51.4128 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 131.1885 to 155.9231 deg, Dec 39.8074 to 51.4128 deg
Loaded 5468 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): 3562 out of 4004 total matches.
Matched with Tycho-2 4004 out of 43830 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits:
Forced-photometry filter: calibrated wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits -> calib.txt_param_ref_wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits (aperture=4.8)
Read 43644 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 131.2455 to 155.9231 deg, Dec +39.8196 to +51.4197 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 131.2455 to 155.9231 deg, Dec 39.8196 to 51.4197 deg
Loaded 5437 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): 3556 out of 4005 total matches.
Matched with Tycho-2 4005 out of 43644 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits:
Forced-photometry filter: calibrated wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits -> calib.txt_param_ref_wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 57 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
2.0 pix UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
2.2 pix fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
2.2 pix fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
1.9 pix wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
2.0 pix wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
Limiting magnitude estimates:
15.7 mag. UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
15.6 mag. UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
14.7 mag. fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
14.7 mag. fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.2 (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.J84s5Nos8V (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.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-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits' -> 'wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
WCS_IMAGE_NAME=wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
WCS-calibrated image found: wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
Checking if the catalog wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat corresponding to the image wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits alredy exist and is non-empty...
Catalog wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat corresponding to the image wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits
WCS catalog name: wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=2151, passed=43815
Got 43815 stars (including 41587 good ones) from the SExtractor catalog wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat
util/solve_plate_with_UCAC5 got 43815 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
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: 975 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 43416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 649 to 709 (Dec 39.8 to 51.4)
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(), 43415 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 43415 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits N_match=975 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.452 sigma_q2_arcsec=0.355 sigma_q3_arcsec=0.339 sigma_q4_arcsec=0.304 n_q1=207 n_q2=259 n_q3=262 n_q4=247 worst_quadrant_to_overall_ratio=1.260
The image catalog is written to wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits -region wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.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.kWWlpmizf0 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.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-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits' -> 'wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
WCS_IMAGE_NAME=wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
WCS-calibrated image found: wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
Checking if the catalog wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat corresponding to the image wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits alredy exist and is non-empty...
Catalog wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat corresponding to the image wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits
WCS catalog name: wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2132, passed=43635
Got 43635 stars (including 41420 good ones) from the SExtractor catalog wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat
util/solve_plate_with_UCAC5 got 43635 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
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: 975 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 43298 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
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(), 43297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 43297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits N_match=975 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.360 sigma_q3_arcsec=0.352 sigma_q4_arcsec=0.272 n_q1=207 n_q2=259 n_q3=262 n_q4=247 worst_quadrant_to_overall_ratio=1.111
The image catalog is written to wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits -region wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.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.kbEzKVwPzW (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_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.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_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
WCS_IMAGE_NAME=wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
WCS-calibrated image found: wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
Checking if the catalog wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat corresponding to the image wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat corresponding to the image wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
WCS catalog name: wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=952, passed=24865
Got 24865 stars (including 23886 good ones) from the SExtractor catalog wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat
util/solve_plate_with_UCAC5 got 24865 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 651 to 708 (Dec 40.4 to 51.3)
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(), 966 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(), 24587 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 651 to 708 (Dec 40.4 to 51.3)
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(), 24587 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 24586 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits N_match=974 sigma_overall_arcsec=0.468 sigma_q1_arcsec=0.316 sigma_q2_arcsec=0.501 sigma_q3_arcsec=0.463 sigma_q4_arcsec=0.565 n_q1=232 n_q2=266 n_q3=241 n_q4=235 worst_quadrant_to_overall_ratio=1.208
The image catalog is written to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits -region wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.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.cRtC329m9U (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_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.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_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
WCS_IMAGE_NAME=wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
WCS-calibrated image found: wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
Checking if the catalog wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat corresponding to the image wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat corresponding to the image wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
WCS catalog name: wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=948, passed=25126
Got 25126 stars (including 24151 good ones) from the SExtractor catalog wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat
util/solve_plate_with_UCAC5 got 25126 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 651 to 708 (Dec 40.4 to 51.3)
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: 975 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 24754 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 651 to 708 (Dec 40.4 to 51.3)
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(), 24753 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 24753 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits N_match=975 sigma_overall_arcsec=0.451 sigma_q1_arcsec=0.342 sigma_q2_arcsec=0.492 sigma_q3_arcsec=0.490 sigma_q4_arcsec=0.541 n_q1=240 n_q2=264 n_q3=235 n_q4=236 worst_quadrant_to_overall_ratio=1.201
The image catalog is written to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits -region wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.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_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-00-25_20.00sec_4.90C_LIGHT_0023.fits
Saving fully-calibrated image wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.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_2026-06-01_CI_UMa-09-Q2b1x1_220532_TTUQ2b1x1_3013292_HkCTgoZ0/wcs_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024.fits
Preparing the HTML report for the field UMa-09-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits at 09:48:31.63 +46:45:06.9: 11.50 +/- 0.00 detection
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits at 09:41:28.73 +44:12:14.0: 13.84 +/- 0.04 detection
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits at 09:48:31.63 +46:45:06.9: 11.45 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.00
Forced photometry filter REJECTED candidate at 09:48:31.63 +46:45:06.9: ref_mag=11.47 +/- 0.00 new_mean_mag=11.8794 delta=-0.41 (need > 0.90)
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits at 09:40:08.94 +45:09:05.9: 14.16 +/- 0.05 detection
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits at 09:41:28.73 +44:12:14.0: 13.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.03
Forced photometry filter REJECTED candidate at 09:41:28.73 +44:12:14.0: ref_mag=13.84 +/- 0.03 new_mean_mag=13.9426 delta=-0.10 (need > 0.90)
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits at 09:53:36.85 +44:40:43.6: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits at 09:37:04.53 +43:21:45.1: 16.31 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits at 09:28:41.82 +41:43:39.1: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits at 09:40:08.94 +45:09:05.9: 14.12 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.03
Forced photometry filter REJECTED candidate at 09:40:08.94 +45:09:05.9: ref_mag=14.14 +/- 0.03 new_mean_mag=14.2125 delta=-0.07 (need > 0.90)
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits at 09:24:17.47 +42:02:20.1: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits at 09:53:36.85 +44:40:43.6: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits at 09:37:04.53 +43:21:45.1: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits at 09:28:41.82 +41:43:39.1: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits at 09:24:17.47 +42:02:20.1: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-44-14_20.00sec_-15.00C_LIGHT_0332.fits at 09:12:28.62 +42:19:07.2: 14.71 +/- 0.09 detection
Forced photometry on wcs_UMa-09-Q2b1x1_2026-01-18_01-45-00_20.00sec_-15.00C_LIGHT_0333.fits at 09:12:28.62 +42:19:07.2: 14.74 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.72 +/- 0.07
Forced photometry filter KEPT candidate at 09:12:28.62 +42:19:07.2: ref_mag=14.72 +/- 0.07 new_mean_mag=13.6582 delta=1.06 (need > 0.90)
Adding exclusion_list_local.txt__out08114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57221.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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: 4s
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Considering the candidate 52413_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 52413_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
**** FOUND 10:00:07.00 +42:15:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52414_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 52414_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
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Considering the candidate 52686_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 52686_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 53067_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 53067_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 53726_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 53726_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
**** FOUND 09:29:07.16 +50:00:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53762_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 53762_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 54009_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 54009_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54043_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 54043_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 54224_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 54224_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 54342_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 54342_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 54653_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 54653_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 54968_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 54968_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 54974_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 54974_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55403_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 55403_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55614_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 55614_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
**** FOUND 09:44:57.57 +43:14:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55666_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 55666_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 55818_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 55818_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 55884_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 55884_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
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Considering the candidate 55911_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 55911_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
**** FOUND 09:50:21.23 +43:59:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55972_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 55972_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 55982_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 55982_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 55984_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 55984_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56064_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 56064_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
**** FOUND 09:29:54.33 +46:11:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56073_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 56073_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56100_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 56100_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
**** FOUND 09:33:42.95 +47:30:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56166_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 56166_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
**** FOUND 09:50:22.52 +43:58:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56339_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 56339_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56397_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 56397_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
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Considering the candidate 56430_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 56430_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56447_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 56447_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56474_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 56474_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56555_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 56555_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 56763_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 56763_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56799_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 56799_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 56805_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 56805_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 56885_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
Preparing report for the candidate 56885_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
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Considering the candidate 56931_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
Preparing report for the candidate 56931_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
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Considering the candidate 56975_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 56975_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 57047_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57047_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 57074_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57074_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 57092_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
Preparing report for the candidate 57092_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
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Considering the candidate 57115_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57115_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57118_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57118_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 57134_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57134_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57148_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57148_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 57163_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57163_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57221_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
Preparing report for the candidate 57221_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
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Considering the candidate 57254_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57254_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 57274_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57274_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 57283_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57283_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 57316_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57316_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57354_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57354_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 57441_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57441_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57454_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57454_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57482_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57482_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 57574_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024
The candidate 57574_fd_UMa-09-Q2b1x1_2026-06-01_22-01-01_20.00sec_4.90C_LIGHT_0024 did not pass the final checks